commit 69717ebdb70089a0fe6196150afeab4e5fd5e253 Author: fengmengqi Date: Thu Mar 19 12:12:32 2026 +0800 first commit diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/AA54562-25.tex b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/AA54562-25.tex new file mode 100644 index 0000000..e32ba63 --- /dev/null +++ b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/AA54562-25.tex @@ -0,0 +1,401 @@ +\documentclass{aa} +\usepackage{lscape} +\usepackage{longtable,threeparttable} +\usepackage{graphicx} +\usepackage{txfonts} +\usepackage{caption} +\usepackage{subcaption} +\usepackage{hyperref} +\usepackage[normalem]{ulem} +\usepackage{soul} +\usepackage{color} +\hypersetup{ + unicode=true, + pdftoolbar=true, + pdfmenubar=true, + pdffitwindow=false, + pdfstartview={FitH}, + pdftitle={My title}, + pdfauthor={Author}, + pdfsubject={Subject}, + pdfcreator={Creator}, + pdfproducer={Producer}, + pdfkeywords={keyword1, key2, key3}, + pdfnewwindow=true, + colorlinks=true, + linkcolor=blue, + citecolor=blue, + filecolor=magenta, + urlcolor=blue +} +\newcommand {\Fig}{Fig\,} + +\begin{document} + + + \title{From Synthetic SEDs to Stellar Origins: A Deep Learning Model for Physical Parameter Retrieval in Hot Subdwarf Stars} + \titlerunning{Deep Learning SED Modeling of Hot Subdwarfs} + + \author{Mengqi Feng\inst{1} + \and + Zhenxin Lei\inst{1}\fnmsep\thanks{e-mail: \href{mailtoleizhenxin2060@163.com} + {leizhenxin2060@163.com}} + \and + Bokai Kou \inst{1} + \and + Yangyang Dong\inst{1} + \and + Ke Hu\inst{1} + \and + Huaping Xiao\inst{1} + \and + Jingkun Zhao\inst{2} + } + + \institute{Key Laboratory of Stars and Interstellar Medium, Xiangtan University, Xiangtan 411105, People's Republic of China. + \and + Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China. + } + + \authorrunning{Feng et al.} + \abstract + % context heading (optional) + {} + % aims heading (mandatory) +{The formation mechanisms of spectrally diverse hot subdwarfs remain unclear. While existing mass distribution analyses suggest additional channels beyond helium white dwarf (He-WD) mergers contribute to He-rich subdwarf formation, these conclusions are constrained by limited sample sizes of mass-measured He-rich objects.} + % methods heading (mandatory) +{We developed a deep leaning model which combines a convolution neural network (CNN) together with a squeeze-and-excitation (SE) block to calculate synthetic spectral energy distributions (SEDs) for 1,012 spectroscopically confirmed hot subdwarfs. Through directly comparison between synthetic SEDs and observed flux density, we derived stellar parameters (mass, radius, luminosity) for unprecedented number size of hot subdwarf stars, enabling more conclusive channel discrimination than prior studies.} + % results heading (mandatory) +{The mass distribution of sdB/sdOB stars confirmed the results from model predictions of binary populations synthesis (BPS). A primary and secondary peak (i.e., around 0.56 and 0.4 ${\rm M}_{\odot}$) is obviously presented in the mass distribution of He-rich hot subdwarf stars. By comparing with the results from the predictions of recent BPS model, it proposed that the merger of two He-WDs could produce most of the observed He-rich hot subdwarf stars, but the mass transfer during the stable Roche lobe overflow (RLOF) phase in binary evolution should be partially conserved.} + % conclusions heading (optional), leave it empty if necessary + {} + {} + + \keywords{(Stars:) subdwarfs; + binaries (including multiple): close; + Stars: evolution; + Stars: fundamental parameters + } + + \maketitle +% +%________________________________________________________________ + +\section{Introduction} +Hot subdwarf stars are positioned between main-sequence (MS) and white dwarf (WD) regions in the Hertzsprung-Russell Diagram (HRD) \citep{1986A&Aheber}. Hot subdwarf stars have very low stellar masses (e.g., 0.5 ${\rm M}_{\odot}$) and thin envelopes ($M_{\text{env}} \le 0.02 M_{\odot}$), but exhibit very high effective temperatures (e.g., $20,000~\mathrm{K} \leq T_{\text{eff}} \leq 70,000~\mathrm{K}$) and large surface gravities (e.g., $5.0 \leq \log g \leq 6.5$). These blue stars have a diversity of atmospheric compositions that could present atmospheres from pure hydrogen (H) to pure helium (He). According to their spectral line features, hot subdwarfs can be classified into sdB, sdO, sdOB, He-sdB, He-sdO, and He-sdOB types \citep{1990_A&AS_moehler,2017_A&A_geier, 2018ApJ...868...70L}. In addition, \citet{2013A&A...551A..31D} designed an MK-like classification scheme by which hot subdwarf stars could be classified in a similar way as normal MS stars (also see \citealt{2021MNRAS.501..623J, 2024PASJ...76.1084Z}). SdB stars are also referred to extreme horizontal branch (EHB) stars due to their location at the bluest end of horizontal branch (HB +). More characteristics of hot subdwarf stars were described in recent excellent reviews of \citet{2009ARA&A..47..211H, 2016PASPHeber}. + +Generally, single stars with such low stellar mass as hot subdwarfs cannot evolve into core He burning or even a late stage within Hubble time. Although formation channels connected with single stars were proposed by several authors (\citealt{1993ApJ...407..649C, 2008A&A...491..253M}), \citet{2020A&A...642A.180P} found that binary interactions are always required in the formation of hot subdwarf stars, including those in wide binary systems. +Furthermore, most of sdB-type hot subdwarfs were found in close binaries \citep{2001MNRASmaxted, 2004Ap&SSnapiwotzki,2011MNRAScopperwheat, 2025A&A...693A.121H}. These results indicate that binary evolution could provide natural explanations for the formation of hot subdwarfs. + +\citet{2002MNRASHan, 2003MNRASHan} investigated the characteristics of hot subdwarfs formed through binary evolution using binary population synthesis (BPS) method. They found that stable Roche lobe overflow (RLOF), common envelope (CE) ejection, and merger of two Helium-white dwarfs (He-WDs) could produce sdB stars in long-period binaries, short-period binaries and single sdB stars, respectively. Most of observed characteristics for sdB stars could be satisfied by their model predictions. \citet{2012MNRASZhang} and \citet{2017ApJ...835..242Z} studied in detail the mergers of two He-WDs and a WD + MS star, respectively. They found that both channels could produce He-rich sdB stars such that their observed features could be satisfied. +In addition, \citet{2022MNRASmiller} proposed that the merger of carbon-oxygen WDs with He WDs could form He-rich hot subdwarfs with atmospheres strongly enriched by carbon and oxygen. Recently, \citet{2021MNRAS.507.4603M} and \citet{2024RAA....24e5003J} proposed that the MS companion of massive WD could survive the type Ia supernova (SN) explosions and become intermediate He-rich hot subdwarf stars if their envelopes are ejected during the explosion. Their model predicted that the peak of mass distribution for survived stars is around 0.4 $\rm M_{\odot}$, which is consistent with the results in \citet{2023ApJLei}. However, the birth rate of this channel would be too low compared to the number of He-rich hot subdwarf stars discovered up to now \citep{2021MNRAS.507.4603M}. \citet{2024ApJ...964...22L} proposed that massive sdO/B stars could be produced from CE ejection process with an asymptotic giant branch (AGB) star. This model could explain the recently discovered sdO binary star SMSS-J1920 \citep{2022MNRAS.515.3370L}, for which strong Ca H and K lines are presented in its spectrum. + +With a large number of new hot subdwarf stars having been discovered using the new data release of spectroscopic surveys \citep{2017OAst...26..164G, 2019MNRAS.486.2169K, 2018ApJ...868...70L, 2019ApJ...881..135L, 2020ApJ...889..117L, 2023ApJ...942..109L, 2019ApJ...881....7L, 2021ApJS..256...28L,2019A&A...630A..80S, 2021MNRAS.501..623J}, also with the help of Gaia mission Early Data Release 3 (Gaia EDR3, \citealt{2021A&A...649A...1G}), \citet{2022A&ACulpan} compiled two catalogs for known hot subdwarf stars and their candidates, respectively (also see the serial studies, \citealt{2017_A&A_geier, 2019A&A...621A..38G, 2020A&A...635A.193G}). The catalog of known hot subdwarfs contains more than 6000 identified hot subdwarf stars, in which more than 3000 stars have atmospheric parameters and 2,700 stars have radial velocities. The candidate catalog contains more than 60,000 objects, which can be used as reliable input catalogs for follow-up analysis with new observed data from spectroscopy. + +Driven by the availability of large observational datasets, machine learning has been extensively applied in astronomical research, including the studies of hot subdwarfs. \citet{2019ApJbu} combined convolution neural network (CNN) with the support vector machine (SVM) to classify hot subdwarf stars in the dataset of Large Sky Area Multi-Fiber Spectroscopic Telescope (LAMOST, \citealt{2012RAA....12.1197C, 2012RAA....12..723Z}). \citet{2022ApJStan} also used CNN to search for hot subdwarf candidates in a larger LAMOST spectra dataset. More recently, \citet{2024PASJliu} applied machine learning method for identification of hot subdwarfs using photometric data, while \citet{2024ApJSchen} constructed a Se-ResNet+SVM model to search for hot subdwarf stars and predicted their atmospheric parameters. + +Despite considerable progress having been made both in simulation and observation of hot subdwarf stars, questions remain regarding the formation channels for those stars. Some notable challenges are from the determination of physical parameters, such as masses, radii, and luminosities, etc. Accurate mass estimation methods include asteroseismology and Eclipse binary. However, their applications are limited by the strict requirements of observed data that only dozens of hot subdwarfs have accurate masses determined by these methods \citep{2012A&AFontaine}. To analyze the mass distribution of hot subdwarfs with different companion types, \citet{2022A&ASchaffenroth} obtained masses, radii, and luminosities for 68 hot subdwarf stars by comparing observed fluxes with synthetic fluxes calculated from SEDs. With the help of these parameters, and with the help of space-based light curves from the Transiting Exoplanet Survey Satellite (TESS, \citealt{2015JATIS...1a4003R}) and the K2 space mission \citep{2014PASP..126..398H}, \citet{2023A&A...673A..90S} further obtained the masses of 27 companions for these hot subdwarf binaries. + +Using a similar method, \citet{2023ApJLei} obtained masses, radii, and luminosities for 664 single-lined hot subdwarfs with the spectra of LAMOST. Based on this large size of sample, they obtained the mass distributions for hot subdwarf stars with different spectral types, and compared them with the results from model predictions. Although the mass distribution of sdB/sdOB stars is consistent with the prevailing model of \citet{2002MNRASHan, 2003MNRASHan}, they found that He-rich hot subdwarf stars have an obviously lower peak of mass distribution (e.g., around 0.42 ${\rm M}_{\odot}$) than model predictions (e.g., 0.5 - 0.6 ${\rm M}_{\odot}$, see \Fig 12 in \citealt{2023ApJLei}). Based on these comparisons, they proposed that besides the two He-WDs merging channel, there should be other important formation channels for He-rich hot subdwarfs. However, only 39 He-rich stars were used in their statistical analysis, and such a small size sample would influence the final conclusions. + +As a further study of \citet{2023ApJLei}, we constructed a deep learning architecture that integrates a CNN with a squeeze-and-excitation (SE) block to calculate the synthetic SEDs for more than 2000 known hot subdwarfs selected in \citet{2022A&ACulpan} with the spectra of LAMOST and Sloan Digital Sky Survey (SDSS, \citealt{2020ApJS..249....3A}). +Using these SEDs, we calculated the synthetic fluxes at stellar surface and compared them with observed fluxes on the Earth to obtain masses, radii, and luminosities for the selected hot subdwarf stars. These parameters were used in following statistical analysis to help us understand the formation of hot subdwarfs more deeply. The structure of this paper is as follows. Sample selection and methods are described in Section 2. Section 3 presents our main results. A detailed discussion for mass distribution with a large size of sample is given in Section 4. A brief summary in Section 5 closed this paper. + +\section{Methodology and sample selection} +\subsection{Deep learning model SENN } + +\begin{figure*} + \centering + \includegraphics[width=0.8\linewidth]{picture/SENN.pdf} + \caption{The structure of deep learning model SENN. See section 2.1 for detailed description. } + \label{Fig 1} +\end{figure*} + +We designed a deep learning model, which integrates a CNN neural network with a SE-block (hereafter SENN), to calculate synthetic SEDs for selected hot subdwarf stars. + +As shown in \Fig \ref{Fig 1}, SENN accepts normalized stellar spectra with a shape of 2,984 $\times$ 1 as inputs, and processes them through a hierarchical architecture to calculate SEDs. The model is comprised of three modules. Initial Feature Embedding Module uses a 1D convolution layer (64 filters, 3 kernels, ReLU activation) to capture local spectral features, and reshape the output into a 64 $\times$ 2982 tensor. The Squeeze-and-Excitation Feature Refinement Module is then employed, in which a global average pooling (GAP) layer compresses global spatial information into a channel-wise descriptor. This descriptor is connected by two dense layers to fully capture channel-wise dependencies and compute channel-specific weights. These weights are then applied to the original feature map, producing the final weighted feature map. Finally, the SED Regression Module is used to flatten the refined features, pass them through a 64-neuron dense layer, and generate SEDs through an output layer. + + The SENN model takes observed spectra as input features and their corresponding synthetic SEDs as training labels. Through training processes, SENN +established a mapping relationship between observed spectra and synthetic SEDs, enabling it to calculated the synthetic SED associated with a given observed spectrum. With these synthetic SED and the observed magnitudes retrieved from virtual observatory (VO), we could calculate the masses, radii and luminosities of hot subdwarf stars reported in \citet{2022A&ACulpan}, if their atmospheric parameters are known (e.g., $T_{\text{eff}}$ and $\log g$. see Section 2.3). + +\subsection{Training dataset} + +In previous studies (\citealt{2018ApJ...868...70L,2019ApJ...881..135L, 2020ApJ...889..117L, 2023ApJ...942..109L}), 950 single-lined hot subdwarf stars were identified with LAMOST spectra. Their atmospheric parameters, i.e., effective temperature ($T_{\text{eff}}$), surface gravity (${\rm log} g$), and logarithmic number ratio of helium to hydrogen ($\log(n_{\text{He}}/n_{\text{H}})$), were determined by fitting H and He profiles with synthetic spectra. The synthetic spectra and SEDs of these stars were generated using \texttt{Synspec} (version~49; \citealt{2007ApJSLanz}) with non-local thermodynamic equilibrium (NLTE) Tlusty atmospheres (version 204; \citealt{2017arXivHubeny}). See \citet{2018ApJ...868...70L} and \citet{2014ASPC..481...95N} for more details about the synthetic spectra and SEDs calculation. + +In this study, synthetic SEDs of 950 stars mentioned above were used as training sample for SENN model. While the observed spectra of these stars were adopted as SENN inputs. 80\% of the selected stars were used as training dataset, while 20\% of them were used as test dataset. + +\subsection{Known hot subdwarfs and their spectra} +\citet{2022A&ACulpan} compiled a catalog of the known hot subdwarf stars which contains 6,616 unique sources collected from literature. In this catalog, it provides atmospheric parameters for 3,087 stars and radial velocities for 2,791 stars. To obtain the observed spectra for these stars, we cross-matched the catalog with the dataset of LAMOST DR11 and SDSS DR18, and then totally obtained 4,289 spectra. After removing duplicated sources +and low quality spectra (e.g., signal-to-noise ratio in the u band less than 5.0 ), 3,411 unique spectra of known hot subdwarfs were left. Since $T_{\text{eff}}$ and $\log g$ are necessary parameters to determine stellar masses and luminosities in this study, only stars with the two parameters reported in the catalog of \cite{2022A&ACulpan} were finally selected for following analysis, and it contains 2047 hot subdwarf stars. + + Within the catalog of \citet{2022A&ACulpan}, the atmospheric parameters of hot subdwarfs were collected from different studies, which predominantly derived through spectral fitting. However, as we lack the specific atmospheric models and parameters used in these works to calculate synthetic spectra for hot subdwarf stars, we did not employ the conventional method of deriving the SEDs for this selected sample with known atmospheric parameters. Instead, we utilized the highly efficient SENN model to compute the SEDs for these hot subdwarfs with corresponding observed spectra. + +Using SENN model constructed in Section 2.1 and the training dataset selected in Section 2.2, synthetic SEDs for 2047 selected hot subdwarf stars were calculated, which will be used to obtain stellar masses, radii, and luminosities in next section. Note that, the SENN model present much higher efficiency on calculating synthetic SEDs when compared with traditional methods. For example, it just need tens of seconds to obtain synthetic SEDs for 2000 stars, and would be more powerful when confronting with huge numbers of stars. + + In Fig \ref{Fig 2}, we compare the ‌synthetic SED of a hot subdwarf star calculated using the ‌SENN model (blue-dashed curve) with that computed directly from ‌Tlusty model (red-solid curve). The near-identical agreement between both SEDs ‌fully demonstrates that utilizing deep learning method to calculate theoretical SEDs for hot subdwarfs is both ‌feasible and reliable. + + +\subsection{Determination of masses, radii, and luminosities for selected hot subdwarf stars} +Using the synthetic SEDs calculated by SENN model, we obtained flux density at the stellar surface within specific pass-band. The synthetic flux density can be compared with the flux density observed on the Earth to determine stellar angular diameters. The synthetic flux density at stellar surface, observed flux density on the Earth, stellar angular diameter, radius and distance of the star have following relationships \citep{2018OAst...27...35H, 2023ApJLei}: +\begin{equation} + \frac{f\left ( \lambda \right ) }{F\left ( \lambda \right ) } =\frac{\theta ^{2} }{4} =\frac{R^{2} }{d^{2}} + \label{eq 1} +\end{equation} + +where $f(\lambda)$ is the flux density observed on the Earth, +$F(\lambda)$ is the synthetic flux density at stellar surface, $\theta$ is angular diameter of the star, $R$ is radius of the star, and $d$ is stellar distance from the Earth. + +If the distance of a star is known, stellar radius can be determined according to Equation (1). Then, with the help of atmospheric parameters (e.g., $\log g$ and $T_{\text{eff}}$), we can obtain mass and luminosity of the star using following equations: + +\begin{align} +M & = \frac{gR^{2}}{G} \label{eq 2} \\ +\frac{L}{L_{\odot} } & = \left ( \frac{R}{R_{\odot}} \right ) ^{2}\left ( \frac{T_{\rm eff}}{T_{\odot}} \right ) ^{4} \label{eq 3} +\end{align} + where $L_{\odot}, R_{\odot}, T_{\odot}$ are luminosity, radius and effective temperature of the Sun. + +Distances for the selected stars in this study were calculated using Gaia DR3 parallaxes \citep{2023A&Agaiadr3} after zero-point correction \citep{2021A&A...649A...4L}. The flux density observed on the Earth were obtained by searching for photometric data using VO SED Analyzer (VOSA, \citealt{2008_A&A_bayo}) of the Spanish Virtual Observatory (SVO) and converting observed magnitudes into fluxes. + + When converting the observed magnitude into the corresponding observed flux on the Earth, an extinction correction must be applied. To determine the visual extinction $A_{\rm V}$, we fitted the synthetic SEDs with the observed fluxes by treating $A_{\rm V}$ as a free parameter. For each trial value of $A_{\rm V}$, the wavelength-dependent extinction $A_\lambda$ was computed as: +\begin{equation} +A_\lambda = A_{\rm V} \times (k_\lambda / k_V), +\end{equation} +where $k_\lambda / k_{\rm V}$ represents the normalized extinction law. The functional form of $k_\lambda / k_V$ was adopted from \citet{1999PASP..111...63F} with $R_{\rm V} = 3.1$ and $k_{\rm V} = 211.4$. The observed fluxes $f_{\text{obs}}(\lambda)$ were then dereddened using: +\begin{equation} +f(\lambda) = f_{\text{obs}}(\lambda) \times 10^{\,A_\lambda / 2.5}, +\end{equation} +which yielding the intrinsic flux density $f(\lambda)$. The best-fit $A_{\rm V}$ were determined simultaneously through $\chi^2$ minimization between the dereddened fluxes and the synthetic SEDs. + +\begin{figure} + \centering + \includegraphics[width=1.0\linewidth]{picture/spec-57919-HD173133N504043V01_sp07-209.fits.pdf} + \caption{Comparison between the synthetic SED calculated with Tlusty model (red-solid curve) and the SED calculated by SENN model (blue-dashed curve). The bottom panel displays the residual differences between the two SEDs.} + \label{Fig 2} +\end{figure} + + Using the method described above, we obtained masses, radii and luminosities for the selected 2,047 hot subdwarf stars. The stars with mass values less than 0.1 $M_\odot$ or larger than 1.0 $M_\odot$ were not reported here, since these values could be significantly influenced by large uncertainties of input parameters, and are not reasonable for normal hot subdwarf stars. Furthermore, only stars with reliable parallaxes (e.g., $\sigma_{\varpi}/\varpi\leq$ 0.2) are included in the following analysis. Thus, we finally have 1,012 hot subdwarf stars with their main parameters reported in this study (see Table \ref{tab1}), which contains 606 sdB, 64 sdO, 206 sdOB, 9 He-sdB, 66 He-sdO, and 61 He-sdOB stars, respectively. The obtained parameter values are presented in Table \ref{tab1}. + + Using Monte Carlo methods, we obtained the statistical errors ($\sigma_{sta}$) for mass, radius, and luminosity of the selected stars. Specifically, we calculated the median values for the three parameters, along with their values at the 16th and 84th percentiles. This defines a 68\% confidence interval around the median values and provides the corresponding asymmetric uncertainties. + + On the other hand, We cross-matched the sample from this work with the sample from \citet{2022A&ASchaffenroth}, and identified 24 common sources. By comparing the masses, radii, and luminosities for these 24 sources, we determined the systematic errors ($\sigma_{sys}$), which were calculated using the following formula: +\begin{equation*} +\sigma_{sys}=\frac{\sum(x_{i}-y_{i}) }{N} +\end{equation*} + where $x_{i}$ is the parameter value calculated in this work, $y_{i}$ is the parameter value calculated in \citet{2022A&ASchaffenroth}, and $N$ is the number of common sources. The final errors ($\sigma$) is then calculated as: + \begin{equation} + \sigma=\sqrt{\sigma_{sta}^2+\sigma_{sys}^2} + \end{equation} + Using the method described above, we obtained systematic errors of ‌0.02 $\rm M_{\odot}$ , ‌0.002 $\rm R_{\odot}$, and ‌1.4 $\rm L_{\odot}$ for mass, radius and luminosity, respectively. In Table \ref{tab1}, we presented the ‌final errors for these three parameters, incorporating both statistical errors and systematic errors. + +\section{Results} +\subsection{Main parameters for selected hot subdwarf stars} + +\begin{figure*} + \centering + \includegraphics[width=0.85\linewidth]{picture/mass_vs_parameters.pdf} + \caption{The relationship between mass and atmospheric parameters for the selected hot subdwarfs. Labels with different colors indicate the spectral classification from \citet{2022A&ACulpan}.} + \label{Fig 3} +\end{figure*} + +The masses, radii, luminosities and other important parameters for the 1,012 selected hot subdwarf stars are presented in Table \ref{tab1}. From left to right, it gives object names, Gaia source\_id, spectral classification, $T_{\text{eff}}$, ${\rm log} g$, extinction coefficient ($A_{\rm V}$), Gaia parallax after zero-point correction, and four parameters obtained in this study, i.e., angular diameter, radius, luminosity and mass. Among these stars, 601 stars have their masses reported in previous studies. It means that the masses of 411 hot subdwarfs were reported for the first time in this study. + +The four panels in \Fig \ref{Fig 3} present the relationships between obtained masses and atmospheric parameters , e.g., from top left to bottom right, it gives planes of mass vs $T_{\text{eff}}$, ${\rm log} g$, $\log (n_{\text{He}}/n_{\text{H}})$ and $\log L$, respectively. It can be observed that most of the selected hot subdwarfs have radii between 0.1 and 0.3 $\rm R_{\odot}$, luminosities between 0.5 and 2.5 $\rm L_{\odot}$, and masses between 0.2 and 0.8 ${\rm M}_{\odot}$, respectively. These results are consistent with those of \citet{2023ApJLei}, also see \Fig 3 in their study. + +\subsection{Comparison with previous study} +In order to evaluate the reliability of the masses, radii, and luminosities obtained in this study, we cross-matched the selected hot subdwarfs with the stars analyzed in \citet{2022A&ASchaffenroth} and \citet{2023ApJLei}, respectively. Comparisons of masses, radii, and luminosities for the common stars are shown in the panels of \Fig \ref{Fig 4}. As can be see in the figure, there is a notable agreement between the results of present study and previous research, particularly with respect to radius and luminosity. However, the comparison of mass exhibits a little larger dispersion than the other two parameters. It is mainly due to the fact that the large uncertainties of surface gravity would directly influence stellar mass determination (see Equation \ref{eq 2}), while it is not used in the determination of radius and luminosity (see Equation \ref{eq 1} and \ref{eq 3}). +\begin{figure*} + \centering + \includegraphics[width=0.3\linewidth]{picture/contrast_Schaffenroth_radius.pdf} + \includegraphics[width=0.3\linewidth]{picture/contrast_Schaffenroth_mass.pdf} + \includegraphics[width=0.3\linewidth]{picture/contrast_Schaffenroth_lumin.pdf} + + \includegraphics[width=0.3\linewidth]{picture/contrast_Lei_radius.pdf} + \includegraphics[width=0.3\linewidth]{picture/contrast_Lei_mass.pdf} + \includegraphics[width=0.3\linewidth]{picture/contrast_Lei_lumin.pdf} + \caption{Top panels: comparison of radii, masses and luminosities between this study and \citet{2022A&ASchaffenroth}. Bottom panels: comparison of radii, masses and luminosities between this study and \citet{2023ApJLei}. } + \label{Fig 4} +\end{figure*} + +\subsection{Mass distribution of hot subdwarf stars} + +\begin{figure*} + \centering + \includegraphics[width=0.45\linewidth]{picture/distribute_mass_plx.pdf} + \includegraphics[width=0.45\linewidth]{picture/distribute_mass_logg.pdf} + \caption{Mass distribution for selected hot subdwarfs with different precisions of parallax (left panel) and surface gravity (right panel). See contexts for details.} + \label{Fig 5} +\end{figure*} + +Since the precision of masses obtained in this study depends mainly on the precision of parallax (i.e., distance) and surface gravity, we showed the mass distribution with different uncertainties of parallax and surface gravity in \Fig \ref{Fig 5}. In the left panel, the entire sample was split into three groups according to the relative parallax uncertainty (e.g., $\sigma_{\varpi}/\varpi\leq$ 0.2, 0.1 and 0.05, respectively). As expected, with the parallax precision increasing from 0.2 to 0.05, the number of hot subdwarf stars in each mass bin decreases. However, the three groups of hot subdwarfs show very similar mass distributions. As can be seen that all groups have a wide mass range of 0.1 - 1.0 ${\rm M}_{\odot}$ and present two distinct peaks: a primary peak at 0.47 ${\rm M}_{\odot}$ and a secondary peak at 0.37 ${\rm M}_{\odot}$ (see detailed discussion on the mass distribution in Section 4). On the other hand, the entire sample was separated into three other groups in the right panel according to the relative uncertainty of surface gravity (e.g., uncertainty of ${\rm log} g$ over ${\rm log} g$ less than 0.09, 0.02 and 0.007, respectively). The three groups in this panel show very similar mass distributions as those in the left panel, which also present two distinct peaks at the same mass values. Considering similar mass distributions for different precisions of parameters, all the selected hot subdwarf stars were adopted in the following analysis. + +\begin{figure} + \centering + \includegraphics[width=1\linewidth]{picture/distribute_mass_spclass.pdf} + \caption{Mass distributions for selected hot subdwarf stars with different spectral classifications.} + \label{Fig 6} +\end{figure} +In \Fig \ref{Fig 6}, we present the mass distributions for hot subdwarf stars according to their spectral classifications, e.g., He-poor sdB/sdOB (red-dashed histogram) , He-rich stars (blue histogram, including He-sdB, He-sdO, and He-sdOB), and He-poor sdO (green histogram). The mass distribution of He-poor sdB/sdOB stars, which make up majority of the hot subdwarf population, closely mirrors that of the entire sample, with two peaks at 0.47 and 0.37 ${\rm M}_{\odot}$. For He-rich hot subdwarfs, two peaks are also present, but the values differ from those seen in sdB/sdOB, occurring at 0.4 and 0.58 ${\rm M}_{\odot}$ (see the discussion in Section 4.3), respectively. However, He-poor sdO stars have a much flatter mass distribution and consist primarily of low-mass stars. + +\section{Discussion} +\subsection{Comparison of mass distribution with previous study.} + +We compared the mass distribution of entire sample with that of \citet{2023ApJLei} in \Fig \ref{Fig 7}. Both two mass distributions exhibit a wide mass range of 0.1 - 1.0 ${\rm M}_{\odot}$. It should be due to the large uncertainties of input parameters (e.g., parallax and surface gravity), which have been used to estimate the mass of hot subdwarf star in both two studies. In general, the two mass distributions show the basic consistency that a primary peak appears around 0.47 ${\rm M}_{\odot}$, and the distribution trend for the low-mass and high-mass sides is nearly the same. As described in Section 3.3, in addition to the primary one, a second mass peak (around 0.37 ${\rm M}_{\odot}$) is also clearly presented in the mass distribution of this study (red histogram). Nevertheless, this distinct feature is much more obscure in the mass distribution of \citet{2023ApJLei} (blue-dashed histogram). Note that, the input surface gravities used to calculate mass for the two studies are from different catalogs. The parameters used in this study are from the catalog of \citet{2022A&ACulpan}, which were collected from other literature \citep{2020A&A...635A.193G, 2021ApJS..256...28L, 2021MNRAS.501..623J}. While the parameters used in \citet{2023ApJLei} are from \citet{2018ApJ...868...70L, 2019ApJ...881..135L, 2020ApJ...889..117L, 2023ApJ...942..109L}. The method of spectral analysis and the observed spectra used in these studies could be different, which would lead to the differences in obtained parameters. For example, the systematic errors of surface gravity between \citet{2021ApJS..256...28L} and Lei et al. are around 0.07 dex. Thus, these differences would cause an inconsistency in the mass distribution, especially for some local features. + +\begin{figure} + \centering + \includegraphics[width=1\linewidth]{picture/distribute_mass_with_previos_work.pdf} + \caption{Comparison of mass distribution between this study (red histogram) and \citet{2023ApJLei} (blue-dashed histogram).} + \label{Fig 7} +\end{figure} + +\subsection{Mass distribution of He-poor sdB/sdOB stars} + +\citet{2003MNRASHan} (hereafter Han03) have carried out a detailed binary population synthesis (BPS) study on the formation of sdB-type hot subdwarfs. In their study, 12 sets of models were constructed with various input parameters to investigate their impacts on the formation of sdB stars. Among these models, the model of set 2 (with $Z=0.02$, a flat initial mass ratio distribution, $q_{\rm crit}$ = 1.5, $\alpha_{\rm CE}$ = $\alpha_{\rm th}$ = 0.75) was chosen as the best-fitting model in their study that could satisfy most of the observed properties for sdB stars. These results from BPS models provide great convenience for direct comparison with observations. + +The left panel of \Fig \ref{Fig 8} exhibits comparisons between the mass distribution of set 2 in Han03 (black solid curve) and that of this study (gray histogram). As discussed in Section 4.1, the mass distribution for sdB/sdOB stars in this study shows a wide mass range from 0.1 to 1.0 ${\rm M}_{\odot}$ due to the large uncertainties of surface gravity and parallax. While the mass distribution of Han03 ranges from 0.3 to 0.8 ${\rm M}_{\odot}$ which is narrower than that of this study. Since the minimum core mass for He ignition is about 0.3 ${\rm M}_{\odot}$ (see Table 1 and 2 in \citealt{2002MNRASHan}), there is a cut off of mass around 0.3 ${\rm M}_{\odot}$ for the low mass side in the distribution of Han03. Therefore, the stars with masses less than 0.3 ${\rm M}_{\odot}$ in this study could be low-mass WDs or extremely low-mass (ELM) WDs (also see the discussion in Section 4.4 of \citealt{2023ApJLei}). + +Furthermore, three distinct peaks are presented in the mass distribution of Han03, e.g., around 0.46, 0.4 and 0.36 ${\rm M}_{\odot}$, which are generated through the combination of the first CE, the second CE and the first stable RLOF channels (see \Fig 12 and Section 7.3 in their study). As can be seen clearly in the panel, the primary mass peak (around 0.47 ${\rm M}_{\odot}$) in our study is consistent very well with the model prediction of Han03. The secondary mass peak in our study (e.g., around 0.36 ${\rm M}_{\odot}$) corresponds to the left mass peak in Han03, which demonstrates that these stars are mainly produced by the stable RLOF channel with their progenitors at Hertzsprung gap evolution stage. On the other hand, the middle mass peak (e.g., around 0.4 ${\rm M}_{\odot}$) in Han03 is obscure in our mass distribution, for which the stars are mainly produced from the first and the second CE channel with the mass of progenitors around 1.9 ${\rm M}_{\odot}$ (see Table 1 in \citealt{2002MNRASHan}). + + +\begin{figure*} + \centering + \includegraphics[width=0.4\linewidth]{picture/distribute_mass_sdB_sdOB_with_hanset2.pdf} + \includegraphics[width=0.4\linewidth]{picture/distribute_mass_sdB_sdOB_with_segovia2024_all.pdf} + \caption{Left panel: comparison of mass distribution for sdB/sdOB stars between this study (gray histogram) and Han03 (black solid curve). Right panel: comparison of mass distribution for sdB/sdOB stars between this study (gray histogram) and \citet{2025PASA...42...12R} (black solid curve).} + \label{Fig 8} +\end{figure*} + +\citet{2025PASA...42...12R} also studied the impacts of various parameters on the formation of sdB stars through BPS methods. Unlike previous BPS models (e.g., Han03, \citealt{2012ApJ...746..186C}), they considered H-rich shells using an analytic prescription in the study which gets more closer to the real evolution of sdB stars. In the right panel of \Fig \ref{Fig 8}, we compared the mass distribution predicted by \citet{2025PASA...42...12R} with that of this study. The mass range of sdB stars predicted by \citet{2025PASA...42...12R} (e.g., shown by black solid curve in the right panel) is roughly from 0.3 to 0.62 ${\rm M}_{\odot}$ and is a little narrower than that of Han03 and this study. Note that the results of two He-WDs merging are not included in the BPS code COMPAS \citep{2022ApJSRiley} that was used in their study \footnote{Although the results of two He-WDs merging are not taken into account in COMPAS, \citet{2025PASA...42...12R} still give a simplified and qualitative analysis on this channel, see Section 3.2.4 in their study and Section 4.3 in this study for details.}, therefore some massive hot subdwarf stars are absent in the mass distribution of \citet{2025PASA...42...12R}. As shown in the panel, a sharp primary peak around 0.47 ${\rm M}_{\odot}$ is clearly presented in both two mass distributions, which indicates good agreement between the predictions of BPS model and observations. Furthermore, a second peak of around 0.37 ${\rm M}_{\odot}$ is also presented in the mass distribution of \citet{2025PASA...42...12R} (Also see Fig 7 in \citealt{2025MNRAS.539.3273R}). Although the relative number of stars around this peak in their study is less than that of present study, it shows a one-to-one correspondence between the two studies. + +\subsection{Mass distribution for He-rich Hot subdwarfs} +Two He-WDs merger is considered as the dominant formation channel for He-rich hot subdwarf stars (e.g., $\log(n{\rm He}/n{\rm H})$ $>$ -1.0). The mass range of He-rich hot subdwarfs produced by this channel in Han03 is roughly from 0.42 to 0.76 ${\rm M}_{\odot}$, with a relatively flat peak between 0.5 and 0.6 ${\rm M}_{\odot}$. \citet{2012MNRASZhang} studied three different merging models for two He-WDs, and found that the results could explain most of observed gravities, effective temperatures and surface chemical abundance for He-rich stars. Furthermore, \citet{2017ApJ...835..242Z} found that the mergers of He-WD with low-mass MS star could contribute to the formation of intermediate He-rich (iHe-rich) hot subdwarfs. On the other hand, \citet{2021MNRAS.507.4603M} proposed that MS companions could survive Ia SN explosions and evolve as He-rich hot subdwarfs (also see \citealt{2024RAA....24e5003J}). They obtained a wide mass range of 0.35 to 1.0 ${\rm M}_{\odot}$ for this formation channel, with a mass peak around 0.4 ${\rm M}_{\odot}$. + +As mentioned above, \citet{2023ApJLei} obtained a wide mass range and sharp mass peak around 0.42 ${\rm M}_{\odot}$ for He-rich hot subdwarf stars observed by LAMOST. The mass peak in their study is much lower than the prediction of Han03 and \citet{2012MNRASZhang}. On the other hand, the mass peak in \citet{2023ApJLei} is basically consistent with the value predicted by \citet{2021MNRAS.507.4603M}, but the birth rate for this channel could be too low to explain the discovered He-rich hot subdwarfs (see Section 4.1 of \citealt{2021MNRAS.507.4603M}). According to these results, \citet{2023ApJLei} proposed that, besides the two He-WDs merger, some other channels could contribute to the formation of He-rich hot subdwarfs. \citet{2024ApJS..271...21L} came into a similar conclusion after analyzing the surface chemical abundances of He-rich hot subdwarf stars. + +\begin{figure*} + \centering + \includegraphics[width=1\linewidth]{picture/distribute_mass_He_rich.pdf} + \caption{Left panel: comparison of mass distribution for He-rich stars between this study (gray histogram) and \citet{2023ApJLei} (red-dotted curve). Middle panel: comparison of mass distribution for He-rich stars between this study and Han03 (black solid curve). Right panel: comparison of mass distribution for He-rich stars between this study and \citet{2025PASA...42...12R} (blue dot-dashed curve). } + \label{Fig 9} +\end{figure*} + +However, due to limited size of the sample analyzed in \citet{2023ApJLei}, e.g., only 39 He-rich stars in group 3 of their sample (see Table 2 in their study), it would influence the statistical results for mass distribution without completeness of sample. Thanks to the deep learning model SENN designed in present study (see Section 2.1), more than 2000 synthetic SEDs of the selected hot subdwarfs were calculated. Using these information, the masses of 131 He-rich stars were determined in this study, with the sample size being much larger than that analyzed in \citet{2023ApJLei}. Therefore, a comparison of the mass distribution between this study and previous studies could help better understand the formation of He-rich hot subdwarf stars. + +In the left panel of \Fig \ref{Fig 9}, we compared the mass distribution of He-rich stars obtained in present study with that of in \citet{2023ApJLei}. As can be seen in the panel, it exhibits a relatively wide mass distribution that is roughly from 0.3 to 0.9 ${\rm M}_{\odot}$ for both two studies (Note that, hot subdwarf stars with mass less than 0.3 ${\rm M}_{\odot}$ cannot be produced in model predictions, thus we cut off these stars in our results for the comparison). Two distinct mass peaks are presented in the mass distribution of this study (gray histogram), e.g., a primary peak around 0.56 ${\rm M}_{\odot}$ and a secondary peak around 0.4 ${\rm M}_{\odot}$. As mentioned above, a sharp mass peak around 0.42 ${\rm M}_{\odot}$ is clearly shown in the mass distribution of \citet{2023ApJLei} (red-dotted curve), which corresponds to the secondary mass peak in this study. However, it could be due to the small sample size used in their study that no distinct mass peak between 0.5 and 0.6 ${\rm M}_{\odot}$ can be distinguished in the mass distribution of \citet{2023ApJLei}. + +In the middle panel of \Fig \ref{Fig 9}, we compared the mass distribution of He-rich stars in this study with that of Han03. As can be seen clearly in the panel, our mass distribution is much wider than that of in Han03 (e.g., roughly from 0.42 to 0.76 ${\rm M}_{\odot}$, black-solid curve). As discussed in Section 4.1, it could be due to large uncertainties of parallax and gravity, which significantly affect the precision of mass determination in this study. He-rich stars produced through two He-WDs merger in Han03 present a flat mass peak between 0.5 and 0.6 ${\rm M}_{\odot}$, which could be roughly corresponding to the primary mass peak around 0.56 ${\rm M}_{\odot}$ in this study. However, the secondary mass peak around 0.4 ${\rm M}_{\odot}$ is not predicted by BPS models of Han03, which would demonstrate that two He-WDs merging channel cannot explain the formation of all He-rich hot subdwarf stars. + +Nevertheless, it leads to a little different conclusion when comparing our results with recent BPS model predictions from \citet{2025PASA...42...12R} (see the right panel in \Fig \ref{Fig 9}). The mass distribution of He-rich stars from merging channel of \citet{2025PASA...42...12R} (blue dot-dashed curve) presents two distinct mass peaks around 0.55 ${\rm M}_{\odot}$ and 0.41 ${\rm M}_{\odot}$ (see \Fig 14 in their study), which gives perfect correspondence to the two peaks shown in our study (gray histogram). However, the relative number of He-rich stars around the secondary mass peak (e.g., 0.41 ${\rm M}_{\odot}$) predicted by \citet{2025PASA...42...12R} is less than in this study. As discussed in Section 3.2.4 of their study, the secondary mass peak heavily depends on mass-transfer accretion efficiency at stable RLOF phase. It would disappear when the accretion efficiency equals 0, and it would merge with the primary peak and form a symmetrical distribution with a peak around 0.47 ${\rm M}_{\odot}$ if the accretion efficiency equals 1. + + Note that the formation of two He-WDs binary \footnote{In \citet{2025PASA...42...12R}, the treatment of two He-WDs merging channel was very sample. They did not evolve the two He-WDs binary into merging phase, instead they considered the binary system as hot subdwarfs if they could merge within the age of our universe (e.g., 14 Gyr).} need two RLOF phases. The whole envelope of the primary star will be removed through stable mass transfer during the first RLOF phase. While the two components will be surrounded by a CE formed due to unstable mass transfer during the second RLOF phase, and the CE should be ejected before the two He-WDs binary is formed \citep{1984ApJ...277..355W}. The mass-transfer accretion efficiency during the first RLOF phase have significant effects on the loss of angular momentum due to mass loss from the system, which in turn determine following evolution of the orbital separation. Therefore, a lower accretion efficiency during the first RLOF phase would result in either systems not triggering CE events (too far from each other) or merging (too close), both resulting in a final configuration different from the two He-WDs binary. + + Based on the discussion mentioned above, if the second mass peak (around 0.4 ${\rm M}_{\odot}$) is a real feature, the two He-WDs merging channel could produce most of the observed He-rich hot subdwarf stars on the condition that mass transfer during the first RLOF phase to produce the two He-WDs binary should be partially conserved, and the accretion efficiency can not be too low. + +\section{Summary} + +In this study, a deep learning model SENN was designed to calculate synthetic SEDs for a large number of known hot subdwarfs with the help of spectra from LAMOST and SDSS. Through VOSA service of Spanish Virtual Observatory, the physical parameters (e.g., masses, radii, and luminosities) of 1,012 hot subdwarfs were obtained by comparing the synthetic SEDs with the observed flux density. With obtained parameters for a large size of sample, comparisons between observations and model predictions would help us understand the formation of hot subdwarf stars more deeply and comprehensively. + +The two mass peaks (e.g., 0.47 and 0.37) in mass distribution of sdB/sdOB stars are consistent with the prediction from BPS models, which corresponds to the production of CE ejection and stable RLOF respectively. There is also a primary peak (around 0.56 ${\rm M}_{\odot}$) and a secondary peak (around 0.4 ${\rm M}_{\odot}$) clearly presented in the mass distribution of He-rich stars. Although the primary mass peak is well predicted by BPS models, occurrence of the secondary peak in the models depends heavily on the mass-transfer accretion efficiency at stable RLOF stage in binary evolution. These results indicate that two He-WDs merging channel could produce most of the observed He-rich hot subdwarf stars, but mass transfer should be partially conserved during the stable RLOF phase. Considering large uncertainties of the masses obtained in this study, other alternative formation channels for He-rich hot subdwarfs would not be completely excluded. More accurate determination of physical parameters for hot subdwarf stars are urgently needed. + +It is important to note that although we could efficiently obtain synthetic SEDs of hot subdwarfs using SENN model, deriving their masses, radii, and luminosities still requires atmospheric parameters ($T_{\text{eff}}$ and ${\rm log} g$). Accurate atmospheric parameters, however, must still be acquired through the conventional method of synthetic spectral fitting.‌ + +Fortunately, we are actively exploring the use of machine learning methods to predict the atmospheric parameters of hot subdwarfs \citep{2026ApJS..283...16L}. This approach, in the near future, should enable us to directly obtain both the atmospheric parameters and masses of hot subdwarfs using artificial intelligence techniques, without having to compute stellar atmosphere models. + +\section{Data availability} + +Table \ref{tab1} is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/. + +\begin{acknowledgements} + + We greatly thank the referee for his/her valuable comments and useful suggestions, which help improve the manuscript significantly. We also thank Nicolás Rodríguez-Segovia for his detailed suggestions on the discussion of Section 4.3. +This work acknowledges support from the National Natural Science Foundation of China (Nos. 12073020, 12588202 and 12273055), Scientific Research Fund of Hunan Provincial Education Department + grant No. 20K124 and 23A0132, the Strategic Priority Research Program of Chinese Academy of Sciences, grant No. XDB1160301. K.H. acknowledges support from the Scientific Research Funds of Hunan Provincial Education Department (Nos. 22A0099 and 24A0101). + This research has made use of the Spanish Virtual Observatory (\url{https://svo.cab.inta-csic.es}) project funded by MCIN/AEI/10.13039/501100011025/ through grant PID2020-112949GB-I00. Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences. +\end{acknowledgements} + +\bibliography{bib} +\bibliographystyle{aa} +\begin{appendix} +\onecolumn +\section{Main parameters for the selected hot subdwarf stars} +\begin{table}[!ht] + \centering + \caption{Main parameters for part of 1,012 selected hot subdwarf stars} + {\fontsize{6}{10}\selectfont + \setlength{\tabcolsep}{2pt} + \begin{tabular}{lllllllllll} + \hline + \centering + Name & \multicolumn{1}{c}{Source\_id} & \multicolumn{1}{c}{sp\_class} & \multicolumn{1}{c}{$T_{\rm eff}$} & \multicolumn{1}{c}{${\rm log} g$} & \multicolumn{1}{c}{$A_{\rm V}$} & \multicolumn{1}{c}{plx\_zp } & \multicolumn{1}{c}{Angular diameter} & \multicolumn{1}{c}{Radius} & \multicolumn{1}{c}{Luminosity} & \multicolumn{1}{c}{Mass} \\ + \multicolumn{1}{c}{} & \multicolumn{1}{c}{Gaia DR3} & \multicolumn{1}{c}{} & \multicolumn{1}{c}{K} & \multicolumn{1}{c}{(cm\ s$^{-2}$)} & \multicolumn{1}{c}{mag} & \multicolumn{1}{c}{mas} & \multicolumn{1}{c}{log(rad)} & \multicolumn{1}{c}{R/R$_{\odot}$} & \multicolumn{1}{c}{L/L$_{\odot}$} & \multicolumn{1}{c}{M/M$_{\odot}$} \\ + \hline + BD+423250 & 2105469320138052864 & sdB & $28700\pm1000$ & $5.08\pm0.02$ & 0.422 & $4.1508\pm0.0319$ & $-10.268^{+0.036}_{-0.020}$ & $0.287^{+0.003}_{-0.003}$ & $50.2^{+7.5}_{-6.8}$ & $0.36^{+0.03}_{-0.03}$ \\ +BD+481777 & 825628714431805056 & sdO & $47565\pm251$ & $5.84\pm0.04$ & 0.010 & $4.2560\pm0.0617$ & $-10.503^{+0.019}_{-0.014}$ & $0.163^{+0.003}_{-0.003}$ & $122.7^{+4.7}_{-4.5}$ & $0.67^{+0.07}_{-0.07}$ \\ +BD-32179 & 3068744791442939904 & sdO & $59121\pm686$ & $4.55\pm0.03$ & 0.010 & $1.0124\pm0.0666$ & $-10.458^{+0.020}_{-0.029}$ & $0.767^{+0.054}_{-0.047}$ & $6445.7^{+992.0}_{-811.9}$ & $0.76^{+0.13}_{-0.10}$ \\ +BPSCS22890-74 & 4420741294390728448 & sdB & $24560\pm567$ & $5.14\pm0.06$ & 1.135 & $1.0170\pm0.0312$ & $-10.690^{+0.064}_{-0.016}$ & $0.430^{+0.014}_{-0.013}$ & $60.4^{+7.1}_{-6.4}$ & $0.93^{+0.15}_{-0.13}$ \\ +Bal90100005 & 2845710850610464640 & sdB & $32789\pm123$ & $5.66\pm0.02$ & 0.302 & $1.2124\pm0.0358$ & $-11.098^{+0.011}_{-0.052}$ & $0.146^{+0.005}_{-0.005}$ & $22.2^{+2.0}_{-1.9}$ & $0.36^{+0.04}_{-0.03}$ \\ +Bal90900004 & 1874534323107953664 & sdB & $42860\pm1590$ & $5.51\pm0.12$ & 0.168 & $1.3991\pm0.0553$ & $-10.883^{+0.018}_{-0.016}$ & $0.207^{+0.009}_{-0.008}$ & $129.9^{+23.4}_{-20.3}$ & $0.51^{+0.17}_{-0.13}$ \\ +CBS250 & 1373881186687373696 & sdB & $32280\pm140$ & $5.76\pm0.03$ & 0.052 & $0.8909\pm0.0328$ & $-11.194^{+0.010}_{-0.007}$ & $0.159^{+0.006}_{-0.006}$ & $24.6^{+2.4}_{-2.2}$ & $0.53^{+0.06}_{-0.05}$ \\ +CBS274 & 1605239049014274560 & sdOB & $36833\pm2000$ & $5.83\pm0.20$ & 0.030 & $0.3374\pm0.0601$ & $-11.708^{+0.014}_{-0.005}$ & $0.128^{+0.028}_{-0.020}$ & $27.3^{+15.3}_{-9.1}$ & $0.41^{+0.34}_{-0.18}$ \\ +CBS282 & 1591755325606144640 & sdOB & $36728\pm932$ & $6.02\pm0.14$ & 0.457 & $0.3160\pm0.0622$ & $-11.696^{+0.024}_{-0.010}$ & $0.139^{+0.034}_{-0.023}$ & $31.5^{+17.6}_{-9.9}$ & $0.75^{+0.53}_{-0.29}$ \\ +CBS374 & 1471988375850922368 & sdOB & $35110\pm73$ & $6.08\pm0.02$ & 0.093 & $1.0166\pm0.0376$ & $-11.195^{+0.025}_{-0.006}$ & $0.139^{+0.006}_{-0.005}$ & $26.3^{+2.5}_{-2.3}$ & $0.85^{+0.08}_{-0.07}$ \\ +CBS98 & 810691780249660800 & sdOB & $33588\pm147$ & $5.39\pm0.03$ & 0.029 & $0.6313\pm0.0665$ & $-11.408^{+0.015}_{-0.008}$ & $0.136^{+0.016}_{-0.013}$ & $21.0^{+5.4}_{-4.1}$ & $0.16^{+0.05}_{-0.04}$ \\ +EGGR113 & 4422600328035803264 & sdO & $61075\pm1182$ & $5.77\pm0.05$ & 0.146 & $0.7145\pm0.0416$ & $-11.398^{+0.005}_{-0.034}$ & $0.124^{+0.008}_{-0.007}$ & $192.9^{+29.2}_{-24.8}$ & $0.33^{+0.06}_{-0.05}$ \\ +FBS0021+418 & 382086995098288896 & sdB & $29032\pm477$ & $5.12\pm0.06$ & 0.224 & $0.3996\pm0.0475$ & $-11.341^{+0.013}_{-0.004}$ & $0.252^{+0.034}_{-0.027}$ & $40.7^{+12.1}_{-8.6}$ & $0.31^{+0.10}_{-0.07}$ \\ +FBS0033+376 & 368263110278860544 & sdB & $38970\pm1330$ & $5.89\pm0.10$ & 0.076 & $1.4164\pm0.0409$ & $-11.144^{+0.008}_{-0.006}$ & $0.112^{+0.004}_{-0.004}$ & $26.2^{+4.3}_{-3.9}$ & $0.36^{+0.10}_{-0.08}$ \\ +FBS0051+377 & 364742852004132736 & sdOB & $35103\pm116$ & $5.91\pm0.02$ & 0.080 & $1.0341\pm0.0418$ & $-11.181^{+0.018}_{-0.006}$ & $0.142^{+0.006}_{-0.006}$ & $27.3^{+2.8}_{-2.5}$ & $0.59^{+0.06}_{-0.06}$ \\ +FBS0102+362 & 369576820516013824 & sdB & $32628\pm98$ & $5.68\pm0.02$ & 0.011 & $2.6839\pm0.0523$ & $-10.729^{+0.007}_{-0.007}$ & $0.154^{+0.004}_{-0.004}$ & $24.1^{+1.7}_{-1.7}$ & $0.41^{+0.03}_{-0.03}$ \\ +FBS0104+367 & 369621277722573568 & sdB & $31086\pm120$ & $5.94\pm0.04$ & 0.157 & $0.7730\pm0.0421$ & $-11.236^{+0.044}_{-0.008}$ & $0.166^{+0.010}_{-0.009}$ & $23.0^{+3.1}_{-2.7}$ & $0.87^{+0.14}_{-0.12}$ \\ +FBS0106+374 & 369573831218501376 & sdB & $30340\pm218$ & $5.75\pm0.05$ & 0.141 & $1.1993\pm0.0391$ & $-10.953^{+0.005}_{-0.006}$ & $0.207^{+0.007}_{-0.007}$ & $32.6^{+2.8}_{-2.6}$ & $0.88^{+0.13}_{-0.11}$ \\ +FBS0117+396 & 371711041304831616 & sdB & $28500\pm100$ & $5.42\pm0.01$ & 0.060 & $0.5853\pm0.0462$ & $-11.279^{+0.035}_{-0.007}$ & $0.198^{+0.017}_{-0.014}$ & $23.3^{+4.4}_{-3.5}$ & $0.38^{+0.07}_{-0.06}$ \\ +FBS0156+439 & 346721341030064640 & He-sdOB & $43970\pm1190$ & $5.72\pm0.16$ & 0.166 & $0.5015\pm0.0491$ & $-11.401^{+0.031}_{-0.009}$ & $0.176^{+0.019}_{-0.016}$ & $103.6^{+26.9}_{-20.1}$ & $0.59^{+0.31}_{-0.20}$ \\ +FBS0203+374 & 330722897089067392 & sdB & $28744\pm303$ & $5.47\pm0.04$ & 0.150 & $1.0701\pm0.0367$ & $-10.984^{+0.044}_{-0.004}$ & $0.214^{+0.008}_{-0.007}$ & $28.0^{+2.7}_{-2.6}$ & $0.49^{+0.06}_{-0.06}$ \\ +FBS0206+428 & 351633546665907200 & sdB & $25735\pm251$ & $5.14\pm0.03$ & 0.135 & $0.9280\pm0.0366$ & $-11.019^{+0.006}_{-0.007}$ & $0.229^{+0.009}_{-0.009}$ & $20.6^{+2.4}_{-2.2}$ & $0.26^{+0.04}_{-0.03}$ \\ +FBS0208+390 & 332606704106366848 & sdB & $38743\pm269$ & $6.15\pm0.04$ & 0.106 & $0.7313\pm0.0419$ & $-11.439^{+0.008}_{-0.011}$ & $0.111^{+0.007}_{-0.006}$ & $24.8^{+3.5}_{-3.0}$ & $0.63^{+0.10}_{-0.09}$ \\ +FBS0212+334 & 326009496898928896 & sdB & $29697\pm197$ & $5.63\pm0.04$ & 0.254 & $1.2116\pm0.0350$ & $-10.875^{+0.012}_{-0.006}$ & $0.243^{+0.007}_{-0.007}$ & $41.3^{+3.0}_{-2.9}$ & $0.92^{+0.11}_{-0.10}$ \\ +FBS0314+372 & 235323736345986176 & sdB & $29283\pm192$ & $5.42\pm0.03$ & 0.902 & $0.8740\pm0.0403$ & $-11.085^{+0.007}_{-0.029}$ & $0.209^{+0.010}_{-0.009}$ & $28.8^{+3.3}_{-2.9}$ & $0.42^{+0.06}_{-0.05}$ \\ +FBS0324+379 & 234861632224343424 & sdB & $24809\pm298$ & $5.27\pm0.03$ & 0.473 & $1.3008\pm0.0340$ & $-10.908^{+0.009}_{-0.007}$ & $0.210^{+0.006}_{-0.006}$ & $15.0^{+1.8}_{-1.7}$ & $0.30^{+0.03}_{-0.03}$ \\ +FBS0638+428 & 963881581386403072 & sdB & $28090\pm161$ & $5.29\pm0.02$ & 0.229 & $1.1992\pm0.0344$ & $-10.985^{+0.042}_{-0.010}$ & $0.191^{+0.006}_{-0.006}$ & $20.4^{+1.9}_{-1.9}$ & $0.26^{+0.03}_{-0.03}$ \\ +FBS0639+391 & 944892878136403712 & sdB & $29658\pm509$ & $5.53\pm0.08$ & 0.372 & $0.8262\pm0.0358$ & $-11.070^{+0.008}_{-0.007}$ & $0.229^{+0.010}_{-0.010}$ & $36.3^{+4.5}_{-4.0}$ & $0.65^{+0.15}_{-0.12}$ \\ +FBS0646+386 & 944390774983674496 & sdB & $33238\pm190$ & $5.63\pm0.03$ & 0.234 & $0.7018\pm0.0473$ & $-11.323^{+0.020}_{-0.012}$ & $0.150^{+0.011}_{-0.010}$ & $24.6^{+3.9}_{-3.4}$ & $0.35^{+0.06}_{-0.05}$ \\ +FBS1400+389 & 1495942160078351744 & sdOB & $18800\pm1000$ & $4.71\pm0.10$ & 0.029 & $1.4515\pm0.0345$ & $-10.534^{+0.020}_{-0.045}$ & $0.449^{+0.011}_{-0.011}$ & $22.6^{+5.5}_{-4.7}$ & $0.38^{+0.10}_{-0.08}$ \\ +FBS1531+381 & 1375814952762454272 & sdB & $29230\pm125$ & $5.58\pm0.03$ & 0.029 & $1.9294\pm0.0345$ & $-10.805^{+0.013}_{-0.164}$ & $0.181^{+0.004}_{-0.004}$ & $21.5^{+1.7}_{-1.6}$ & $0.46^{+0.04}_{-0.04}$ \\ +FBS1715+424 & 1360139937040515072 & sdO & $58438\pm514$ & $6.11\pm0.03$ & 0.010 & $2.3950\pm0.0387$ & $-10.911^{+0.011}_{-0.009}$ & $0.114^{+0.003}_{-0.003}$ & $135.4^{+6.8}_{-6.4}$ & $0.61^{+0.05}_{-0.05}$ \\ +FBS1745+437 & 1349088676950060672 & sdB & $33601\pm109$ & $5.56\pm0.02$ & 0.073 & $1.0659\pm0.0262$ & $-11.132^{+0.008}_{-0.006}$ & $0.153^{+0.004}_{-0.004}$ & $26.9^{+2.0}_{-1.9}$ & $0.31^{+0.03}_{-0.03}$ \\ +FBS2255+404 & 1930945626165804032 & He-sdOB & $48127\pm277$ & $5.92\pm0.04$ & 0.355 & $0.4056\pm0.0444$ & $-11.490^{+0.049}_{-0.010}$ & $0.176^{+0.022}_{-0.017}$ & $149.9^{+39.4}_{-28.1}$ & $0.95^{+0.27}_{-0.19}$ \\ +FBS2307+338 & 1911572540520290048 & He-sdO & $50664\pm390$ & $5.85\pm0.04$ & 0.219 & $0.4957\pm0.0502$ & $-11.435^{+0.006}_{-0.011}$ & $0.165^{+0.018}_{-0.015}$ & $160.2^{+38.3}_{-28.2}$ & $0.70^{+0.18}_{-0.14}$ \\ +FBS2347+385 & 2881551562420806784 & sdB & $23770\pm350$ & $5.38\pm0.06$ & 0.269 & $3.9390\pm0.0341$ & $-10.434^{+0.026}_{-0.011}$ & $0.207^{+0.003}_{-0.003}$ & $12.3^{+1.6}_{-1.6}$ & $0.37^{+0.06}_{-0.05}$ \\ +Feige114 & 1858674589447492608 & sdOB & $37689\pm189$ & $5.56\pm0.02$ & 0.148 & $1.2354\pm0.0317$ & $-10.983^{+0.023}_{-0.006}$ & $0.186^{+0.005}_{-0.005}$ & $62.5^{+3.8}_{-3.6}$ & $0.46^{+0.04}_{-0.04}$ \\ +Feige26 & 2503706418759709184 & He-sdO & $65608\pm912$ & $5.46\pm0.04$ & 0.010 & $0.5763\pm0.0471$ & $-11.247^{+0.007}_{-0.010}$ & $0.218^{+0.019}_{-0.017}$ & $793.7^{+154.1}_{-121.7}$ & $0.50^{+0.11}_{-0.09}$ \\ +Feige34 & 781164326766404736 & sdO & $62400\pm330$ & $5.95\pm0.02$ & 0.145 & $4.4105\pm0.1039$ & $-10.645^{+0.069}_{-0.018}$ & $0.113^{+0.003}_{-0.003}$ & $174.4^{+9.3}_{-8.8}$ & $0.42^{+0.04}_{-0.03}$ \\ +Feige67 & 3935488605023787392 & sdO & $61114\pm318$ & $5.92\pm0.01$ & 0.105 & $2.9833\pm0.0735$ & $-10.739^{+0.010}_{-0.039}$ & $0.136^{+0.004}_{-0.004}$ & $232.9^{+13.0}_{-12.0}$ & $0.56^{+0.04}_{-0.04}$ \\ +GALEXJ00468+1956 & 2801277176253968640 & sdB & $32891\pm111$ & $5.84\pm0.02$ & 0.200 & $0.9281\pm0.0413$ & $-11.213^{+0.041}_{-0.008}$ & $0.146^{+0.007}_{-0.006}$ & $22.2^{+2.5}_{-2.3}$ & $0.53^{+0.06}_{-0.05}$ \\ +GALEXJ00476+3123 & 360511037906831872 & sdB & $31069\pm166$ & $5.65\pm0.03$ & 0.207 & $1.0593\pm0.0383$ & $-11.149^{+0.042}_{-0.011}$ & $0.148^{+0.006}_{-0.006}$ & $18.4^{+2.0}_{-1.9}$ & $0.36^{+0.04}_{-0.04}$ \\ +GALEXJ00498+3522 & 363795760175504768 & sdOB & $36551\pm243$ & $5.74\pm0.04$ & 0.063 & $0.8767\pm0.0412$ & $-11.251^{+0.010}_{-0.016}$ & $0.142^{+0.007}_{-0.007}$ & $32.5^{+3.7}_{-3.3}$ & $0.41^{+0.06}_{-0.05}$ \\ +GALEXJ01012+3125 & 312628749626419328 & sdB & $28202\pm155$ & $5.45\pm0.02$ & 0.063 & $1.8070\pm0.0362$ & $-10.788^{+0.010}_{-0.017}$ & $0.201^{+0.005}_{-0.004}$ & $22.9^{+1.8}_{-1.7}$ & $0.41^{+0.03}_{-0.03}$ \\ +GALEXJ01194+4901 & 400211958948711552 & He-sdOB & $43720\pm510$ & $5.86\pm0.21$ & 0.313 & $1.2614\pm0.0326$ & $-10.965^{+0.017}_{-0.012}$ & $0.189^{+0.005}_{-0.005}$ & $117.7^{+8.6}_{-8.0}$ & $0.95^{+0.59}_{-0.37}$ \\ +GALEXJ01509+3107 & 304311150320629376 & sdB & $30183\pm189$ & $5.84\pm0.04$ & 0.130 & $1.3955\pm0.0367$ & $-11.041^{+0.004}_{-0.008}$ & $0.145^{+0.004}_{-0.004}$ & $15.6^{+1.7}_{-1.7}$ & $0.53^{+0.06}_{-0.06}$ \\ +GALEXJ01543+4905 & 357580873780641920 & sdB & $32100\pm410$ & $5.50\pm0.32$ & 0.452 & $1.7860\pm0.0250$ & $-10.871^{+0.008}_{-0.008}$ & $0.166^{+0.003}_{-0.003}$ & $26.4^{+2.1}_{-2.1}$ & $0.32^{+0.35}_{-0.17}$ \\ +GALEXJ02069+1438 & 77515058657678592 & sdB & $30310\pm660$ & $5.77\pm0.06$ & 0.132 & $2.2104\pm0.0447$ & $-10.881^{+0.010}_{-0.028}$ & $0.133^{+0.003}_{-0.003}$ & $13.3^{+1.9}_{-1.9}$ & $0.38^{+0.06}_{-0.05}$ \\ +GALEXJ02163+2759 & 107585292928397568 & sdB & $25480\pm450$ & $5.35\pm0.05$ & 0.155 & $1.5540\pm0.0313$ & $-10.767^{+0.028}_{-0.013}$ & $0.244^{+0.005}_{-0.005}$ & $22.5^{+2.4}_{-2.3}$ & $0.49^{+0.07}_{-0.06}$ \\ +GALEXJ02328+4411 & 341195058150383104 & sdB & $33260\pm420$ & $5.73\pm0.10$ & 0.237 & $1.2611\pm0.0577$ & $-11.082^{+0.011}_{-0.007}$ & $0.145^{+0.007}_{-0.007}$ & $23.1^{+2.9}_{-2.7}$ & $0.41^{+0.12}_{-0.09}$ \\ +GALEXJ04158+0154 & 3259060049366022400 & sdBV & $34773\pm123$ & $5.79\pm0.02$ & 0.359 & $1.5335\pm0.0402$ & $-11.003^{+0.014}_{-0.006}$ & $0.144^{+0.004}_{-0.004}$ & $27.1^{+2.1}_{-2.0}$ & $0.46^{+0.04}_{-0.04}$ \\ +GALEXJ04205+0120 & 3255780171819962496 & He-sdO & $46050\pm910$ & $5.97\pm0.16$ & 0.081 & $2.4658\pm0.0620$ & $-10.816^{+0.012}_{-0.006}$ & $0.137^{+0.004}_{-0.004}$ & $76.2^{+7.5}_{-6.9}$ & $0.64^{+0.29}_{-0.20}$ \\ +GALEXJ04593-0228 & 3225359193340812288 & sdB & $30613\pm608$ & $5.70\pm0.12$ & 0.062 & $1.1390\pm0.0412$ & $-11.197^{+0.033}_{-0.008}$ & $0.124^{+0.005}_{-0.005}$ & $12.0^{+2.0}_{-1.9}$ & $0.28^{+0.09}_{-0.07}$ \\ +GALEXJ05369+3955 & 190970433715259904 & He-sdOB & $38898\pm169$ & $5.79\pm0.04$ & 0.507 & $1.3436\pm0.0332$ & $-11.007^{+0.006}_{-0.008}$ & $0.164^{+0.005}_{-0.004}$ & $55.1^{+3.3}_{-3.1}$ & $0.60^{+0.07}_{-0.06}$ \\ +GALEXJ05557+6408 & 287018271958898560 & sdO & $45600\pm3380$ & $5.73\pm0.39$ & 0.462 & $1.9389\pm0.0248$ & $-10.932^{+0.007}_{-0.023}$ & $0.134^{+0.003}_{-0.003}$ & $70.1^{+23.2}_{-18.7}$ & $0.35^{+0.51}_{-0.21}$ \\ +GALEXJ06134+3420 & 3452237404778065152 & sdOB & $34250\pm390$ & $5.75\pm0.10$ & 0.432 & $1.7373\pm0.0329$ & $-10.935^{+0.010}_{-0.010}$ & $0.148^{+0.003}_{-0.003}$ & $27.1^{+2.2}_{-2.1}$ & $0.45^{+0.12}_{-0.10}$ \\ +GALEXJ063952.00+515658.00 & 992534888766785024 & sdB & $30400\pm340$ & $5.58\pm0.13$ & 0.065 & $3.0845\pm0.0455$ & $-10.552^{+0.031}_{-0.006}$ & $0.202^{+0.004}_{-0.004}$ & $31.2^{+2.2}_{-2.1}$ & $0.56^{+0.20}_{-0.15}$ \\ +GALEXJ06437+3201 & 937248901501446272 & sdB & $26956\pm303$ & $5.12\pm0.04$ & 0.331 & $1.0644\pm0.0448$ & $-10.873^{+0.061}_{-0.008}$ & $0.276^{+0.012}_{-0.011}$ & $36.0^{+3.9}_{-3.5}$ & $0.37^{+0.05}_{-0.05}$ \\ +GALEXJ06463+2920 & 3386622158606040960 & sdOB & $41489\pm229$ & $6.16\pm0.03$ & 0.073 & $2.1178\pm0.0437$ & $-10.998^{+0.009}_{-0.016}$ & $0.105^{+0.003}_{-0.003}$ & $29.3^{+2.0}_{-1.9}$ & $0.58^{+0.05}_{-0.05}$ \\ +GALEXJ07013+5329 & 981727582818800128 & He-sdO & $67230\pm3880$ & $5.60\pm0.22$ & 0.117 & $0.3925\pm0.0431$ & $-11.375^{+0.012}_{-0.005}$ & $0.238^{+0.029}_{-0.023}$ & $1038.8^{+393.0}_{-282.0}$ & $0.83^{+0.61}_{-0.35}$ \\ +GALEXJ07104+2333 & 3368383116127317120 & sdB & $55420\pm24300$ & $5.21\pm0.43$ & 0.724 & $0.5599\pm0.0242$ & $-11.119^{+0.071}_{-0.016}$ & $0.299^{+0.013}_{-0.013}$ & $756.7^{+2464.1}_{-679.2}$ & $0.53^{+0.90}_{-0.33}$ \\ +GALEXJ07108+5624 & 988436459174352512 & sdB & $39970\pm980$ & $5.91\pm0.14$ & 0.094 & $0.9733\pm0.0521$ & $-11.251^{+0.009}_{-0.005}$ & $0.128^{+0.007}_{-0.007}$ & $37.5^{+6.1}_{-5.2}$ & $0.49^{+0.20}_{-0.14}$ \\ +GALEXJ07248+1923 & 3362730178953977472 & sdB & $25777\pm334$ & $5.25\pm0.03$ & 0.172 & $0.9219\pm0.0378$ & $-11.069^{+0.010}_{-0.006}$ & $0.205^{+0.009}_{-0.008}$ & $16.7^{+2.2}_{-2.1}$ & $0.27^{+0.04}_{-0.04}$ \\ + \hline + \end{tabular}} + \label{tab1} +\end{table} + +\end{appendix} +\end{document} diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa.bst b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa.bst new file mode 100644 index 0000000..4abd9a5 --- /dev/null +++ b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa.bst @@ -0,0 +1,1695 @@ +%% 2001/06/10 EDP Sciences +%% APJ, corrected by hand to get results for A&A, using Natbib + +%% 1998/08/12 J Baker +%% Tweaked by hand to get correct results for ApJ. Added functions from +%% astrobib. + +%% $Log: apj.bst,v $ +%% Revision 1.3 2000/04/20 22:17:50 jbaker +%% Fixed INBOOK bug, now works essentially like BOOK. +%% +%% Revision 1.2 1998/08/30 22:35:45 jbaker +%% Added RCS keywords. +%% + +%% +%% This is file `apj.bst', +%% generated with the docstrip utility. +%% +%% The original source files were: +%% +%% merlin.mbs (with options: `,ay,nat,nm-rev,nmdash,dt-beg,yr-per,note-yr,atit-u,jtit-x,jttl-rm,thtit-a,vnum-x,volp-com,jpg-1,pp-last,btit-rm,add-pub,pub-par,pre-edn,edby,edbyx,blk-com,fin-bare,ppx,ed,abr,ord,jabr,eprint,amper,em-x') +%% ---------------------------------------- +%% *** Bibliographic Style for ApJ *** +%% + %------------------------------------------------------------------- + % The original source file contains the following version information: + % \ProvidesFile{merlin.mbs}[1998/02/25 3.85a (PWD)] + % + % NOTICE: + % This file may be used for non-profit purposes. + % It may not be distributed in exchange for money, + % other than distribution costs. + % + % The author provides it `as is' and does not guarantee it in any way. + % + % Copyright (C) 1994-98 Patrick W. Daly + %------------------------------------------------------------------- + % For use with BibTeX version 0.99a or later + %------------------------------------------------------------------- + % This bibliography style file is intended for texts in ENGLISH + % This is an author-year citation style bibliography. As such, it is + % non-standard LaTeX, and requires a special package file to function properly. + % Such a package is natbib.sty by Patrick W. Daly + % The form of the \bibitem entries is + % \bibitem[Jones et al.(1990)]{key}... + % \bibitem[Jones et al.(1990)Jones, Baker, and Smith]{key}... + % The essential feature is that the label (the part in brackets) consists + % of the author names, as they should appear in the citation, with the year + % in parentheses following. There must be no space before the opening + % parenthesis! + % With natbib v5.3, a full list of authors may also follow the year. + % In natbib.sty, it is possible to define the type of enclosures that is + % really wanted (brackets or parentheses), but in either case, there must + % be parentheses in the label. + % The \cite command functions as follows: + % \citet{key} ==>> Jones et al. (1990) + % \citet*{key} ==>> Jones, Baker, and Smith (1990) + % \citep{key} ==>> (Jones et al., 1990) + % \citep*{key} ==>> (Jones, Baker, and Smith, 1990) + % \citep[chap. 2]{key} ==>> (Jones et al., 1990, chap. 2) + % \citep[e.g.][]{key} ==>> (e.g. Jones et al., 1990) + % \citep[e.g.][p. 32]{key} ==>> (e.g. Jones et al., p. 32) + % \citeauthor{key} ==>> Jones et al. + % \citeauthor*{key} ==>> Jones, Baker, and Smith + % \citeyear{key} ==>> 1990 + %--------------------------------------------------------------------- + +ENTRY + { address + archiveprefix %EDP Sciences le 30/11/2014 + author + booktitle + chapter + edition + editor + howpublished + institution + eprint %EDP Sciences le 30/11/2014 + journal + key + month + note + number + organization + pages + publisher + school + series + title + type + volume + year + } + {} + { label extra.label sort.label short.list } + +INTEGERS { output.state before.all mid.sentence after.sentence after.block } + +FUNCTION {init.state.consts} +{ #0 'before.all := + #1 'mid.sentence := + #2 'after.sentence := + #3 'after.block := +} + +STRINGS { s t } + +FUNCTION {output.nonnull} +{ 's := + output.state mid.sentence = + { ", " * write$ } + { output.state after.block = + { add.period$ write$ + newline$ + "\newblock " write$ + } + { output.state before.all = + 'write$ + { add.period$ " " * write$ } + if$ + } + if$ + mid.sentence 'output.state := + } + if$ + s +} + +%EDP Sciences le 30/11/2014 +FUNCTION {output.eprint} +{ 's := + output.state mid.sentence = + { " " * write$ } + { output.state after.block = + { add.period$ write$ + newline$ + "\newblock " write$ + } + { output.state before.all = + 'write$ + { add.period$ " " * write$ } + if$ + } + if$ + mid.sentence 'output.state := + } + if$ + s +} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +FUNCTION {output} +{ duplicate$ empty$ + 'pop$ + 'output.nonnull + if$ +} + +%EDP Sciences le 30/11/2014 +FUNCTION {outputeprint} +{ duplicate$ empty$ + 'pop$ + 'output.eprint + if$ +} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +FUNCTION {output.check} +{ 't := + duplicate$ empty$ + { pop$ "empty " t * " in " * cite$ * warning$ } + 'output.nonnull + if$ +} + +FUNCTION {fin.entry} +{ duplicate$ empty$ + 'pop$ + 'write$ + if$ + newline$ +} + +FUNCTION {new.block} +{ output.state before.all = + 'skip$ + { after.block 'output.state := } + if$ +} + +FUNCTION {new.sentence} +{ output.state after.block = + 'skip$ + { output.state before.all = + 'skip$ + { after.sentence 'output.state := } + if$ + } + if$ +} + +FUNCTION {add.blank} +{ " " * before.all 'output.state := +} + +FUNCTION {date.block} +{ + skip$ +} + +FUNCTION {not} +{ { #0 } + { #1 } + if$ +} + +FUNCTION {and} +{ 'skip$ + { pop$ #0 } + if$ +} + +FUNCTION {or} +{ { pop$ #1 } + 'skip$ + if$ +} + +FUNCTION {new.block.checkb} +{ empty$ + swap$ empty$ + and + 'skip$ + 'new.block + if$ +} + +FUNCTION {field.or.null} +{ duplicate$ empty$ + { pop$ "" } + 'skip$ + if$ +} + +FUNCTION {emphasize} +{ skip$ } + +FUNCTION {capitalize} +{ "u" change.case$ "t" change.case$ } + +FUNCTION {space.word} +{ " " swap$ * " " * } + + % Here are the language-specific definitions for explicit words. + % Each function has a name bbl.xxx where xxx is the English word. + % The language selected here is ENGLISH +FUNCTION {bbl.and} +{ "and"} + +FUNCTION {bbl.editors} +{ "eds." } + +FUNCTION {bbl.editor} +{ "ed." } + +FUNCTION {bbl.edby} +{ "edited by" } + +FUNCTION {bbl.edition} +{ "edn." } + +FUNCTION {bbl.volume} +{ "Vol." } + +FUNCTION {bbl.of} +{ "of" } + +FUNCTION {bbl.number} +{ "no." } + +FUNCTION {bbl.nr} +{ "no." } + +FUNCTION {bbl.in} +{ "in" } + +FUNCTION {bbl.pages} +{ "" } + +FUNCTION {bbl.page} +{ "" } + +FUNCTION {bbl.chapter} +{ "Ch." } +%{ "chap." } + +FUNCTION {bbl.techrep} +{ "Tech. Rep." } + +FUNCTION {bbl.mthesis} +{ "Master's thesis" } + +FUNCTION {bbl.phdthesis} +{ "PhD thesis" } + +FUNCTION {bbl.first} +{ "1st" } + +FUNCTION {bbl.second} +{ "2nd" } + +FUNCTION {bbl.third} +{ "3rd" } + +FUNCTION {bbl.fourth} +{ "4th" } + +FUNCTION {bbl.fifth} +{ "5th" } + +FUNCTION {bbl.st} +{ "st" } + +FUNCTION {bbl.nd} +{ "nd" } + +FUNCTION {bbl.rd} +{ "rd" } + +FUNCTION {bbl.th} +{ "th" } + +MACRO {jan} {"Jan."} + +MACRO {feb} {"Feb."} + +MACRO {mar} {"Mar."} + +MACRO {apr} {"Apr."} + +MACRO {may} {"May"} + +MACRO {jun} {"Jun."} + +MACRO {jul} {"Jul."} + +MACRO {aug} {"Aug."} + +MACRO {sep} {"Sep."} + +MACRO {oct} {"Oct."} + +MACRO {nov} {"Nov."} + +MACRO {dec} {"Dec."} + +FUNCTION {eng.ord} +{ duplicate$ "1" swap$ * + #-2 #1 substring$ "1" = + { bbl.th * } + { duplicate$ #-1 #1 substring$ + duplicate$ "1" = + { pop$ bbl.st * } + { duplicate$ "2" = + { pop$ bbl.nd * } + { "3" = + { bbl.rd * } + { bbl.th * } + if$ + } + if$ + } + if$ + } + if$ +} + +MACRO {acmcs} {"ACM Comput. Surv."} + +MACRO {acta} {"Acta Inf."} + +MACRO {cacm} {"Commun. ACM"} + +MACRO {ibmjrd} {"IBM J. Res. Dev."} + +MACRO {ibmsj} {"IBM Syst.~J."} + +MACRO {ieeese} {"IEEE Trans. Softw. Eng."} + +MACRO {ieeetc} {"IEEE Trans. Comput."} + +MACRO {ieeetcad} + {"IEEE Trans. Comput.-Aided Design Integrated Circuits"} + +MACRO {ipl} {"Inf. Process. Lett."} + +MACRO {jacm} {"J.~ACM"} + +MACRO {jcss} {"J.~Comput. Syst. Sci."} + +MACRO {scp} {"Sci. Comput. Programming"} + +MACRO {sicomp} {"SIAM J. Comput."} + +MACRO {tocs} {"ACM Trans. Comput. Syst."} + +MACRO {tods} {"ACM Trans. Database Syst."} + +MACRO {tog} {"ACM Trans. Gr."} + +MACRO {toms} {"ACM Trans. Math. Softw."} + +MACRO {toois} {"ACM Trans. Office Inf. Syst."} + +MACRO {toplas} {"ACM Trans. Prog. Lang. Syst."} + +MACRO {tcs} {"Theoretical Comput. Sci."} + +INTEGERS { nameptr namesleft numnames } + +FUNCTION {format.names} +{ 's := + #1 'nameptr := + s num.names$ 'numnames := + numnames 'namesleft := + { namesleft #0 > } + { s nameptr + "{vv~}{ll}{, jj}{, f.}" format.name$ + 't := + +numnames #5 > + { + nameptr #1 > + { + nameptr #4 = + { + ", {et~al.}" * + } + { + nameptr #4 > + { "" * } + { ", " * t * } + if$ + } + if$ + + } + 't + if$ + } + { + nameptr #1 > + { + namesleft #1 > + { ", " * t * } + { + numnames #2 > + { "," * } + 'skip$ + if$ + s nameptr "{ll}" format.name$ duplicate$ "others" = + { 't := } + { pop$ } + if$ + t "others" = + { + " {et~al.}" * + } + { " \& " * t * } + if$ + } + if$ + } + 't + if$ + } if$ + + nameptr #1 + 'nameptr := + namesleft #1 - 'namesleft := + } + while$ +} + +FUNCTION {format.names.ed} +{ 's := + #1 'nameptr := + s num.names$ 'numnames := + numnames 'namesleft := + { namesleft #0 > } + { s nameptr + "{f.~}{vv~}{ll}{, jj}" + format.name$ + 't := + nameptr #1 > + { + namesleft #1 > + { ", " * t * } + { + numnames #2 > + { "," * } + 'skip$ + if$ + s nameptr "{ll}" format.name$ duplicate$ "others" = + { 't := } + { pop$ } + if$ + t "others" = + { + " {et~al.}" * + } + { " \& " * t * } + if$ + } + if$ + } + 't + if$ + nameptr #1 + 'nameptr := + namesleft #1 - 'namesleft := + } + while$ +} + +FUNCTION {format.key} +{ empty$ + { key field.or.null } + { "" } + if$ +} + +FUNCTION {format.authors} +{ author empty$ + { "" } + { author format.names } + if$ +} + +FUNCTION {format.editors} +{ editor empty$ + { "" } + { editor format.names + editor num.names$ #1 > + { ", " * bbl.editors * } + { ", " * bbl.editor * } + if$ + } + if$ +} + +FUNCTION {format.in.editors} +{ editor empty$ + { "" } + { editor format.names.ed + } + if$ +} + +FUNCTION {format.note} +{ note empty$ + { "" } + { note #1 #1 substring$ + duplicate$ "{" = + 'skip$ + { output.state mid.sentence = + { "l" } + { "u" } + if$ + change.case$ + } + if$ + note #2 global.max$ substring$ * + } + if$ +} + +%EDP Sciences le 30/11/2014 +FUNCTION {format.eprint} +{ eprint duplicate$ empty$ + 'skip$ + { "[\eprint" + archiveprefix empty$ + 'skip$ + { "[" * archiveprefix * "]" * } + if$ + "{" * swap$ * "}]" * + } + if$ +} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +FUNCTION {format.title} +{ title empty$ + { "" } + { title + } + if$ +} + +FUNCTION {format.full.names} +{'s := + #1 'nameptr := + s num.names$ 'numnames := + numnames 'namesleft := + { namesleft #0 > } + { s nameptr + "{vv~}{ll}" format.name$ + 't := + nameptr #1 > + { + namesleft #1 > + { ", " * t * } + { + numnames #2 > + { "," * } + 'skip$ + if$ + s nameptr "{ll}" format.name$ duplicate$ "others" = + { 't := } + { pop$ } + if$ + t "others" = + { + " {et~al.}" * + } + { " \& " * t * } + if$ + } + if$ + } + 't + if$ + nameptr #1 + 'nameptr := + namesleft #1 - 'namesleft := + } + while$ +} + +FUNCTION {author.editor.key.full} +{ author empty$ + { editor empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { editor format.full.names } + if$ + } + { author format.full.names } + if$ +} + +FUNCTION {author.key.full} +{ author empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { author format.full.names } + if$ +} + +FUNCTION {editor.key.full} +{ editor empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { editor format.full.names } + if$ +} + +FUNCTION {make.full.names} +{ type$ "book" = + type$ "inbook" = + or + 'author.editor.key.full + { type$ "proceedings" = + 'editor.key.full + 'author.key.full + if$ + } + if$ +} + +FUNCTION {output.bibitem} +{ newline$ + "\bibitem[{" write$ + label write$ + ")" make.full.names duplicate$ short.list = + { pop$ } + { * } + if$ + "}]{" * write$ + cite$ write$ + "}" write$ + newline$ + "" + before.all 'output.state := +} + +FUNCTION {n.dashify} +{ + 't := + "" + { t empty$ not } + { t #1 #1 substring$ "-" = + { t #1 #2 substring$ "--" = not + { "--" * + t #2 global.max$ substring$ 't := + } + { { t #1 #1 substring$ "-" = } + { "-" * + t #2 global.max$ substring$ 't := + } + while$ + } + if$ + } + { t #1 #1 substring$ * + t #2 global.max$ substring$ 't := + } + if$ + } + while$ +} + +FUNCTION {word.in} +{ bbl.in + " " * } + +FUNCTION {format.date} +{ year duplicate$ empty$ + { "empty year in " cite$ * "; set to ????" * warning$ + pop$ "????" } + 'skip$ + if$ + extra.label * + before.all 'output.state := + after.sentence 'output.state := +} + +FUNCTION {format.btitle} +{ title +} + +FUNCTION {tie.or.space.connect} +{ duplicate$ text.length$ #3 < + { "~" } + { " " } + if$ + swap$ * * +} + +FUNCTION {either.or.check} +{ empty$ + 'pop$ + { "can't use both " swap$ * " fields in " * cite$ * warning$ } + if$ +} + +FUNCTION {format.bvolume} +{ volume empty$ + { "" } + { bbl.volume volume tie.or.space.connect + series empty$ + 'skip$ + { bbl.of space.word * series emphasize * } + if$ + "volume and number" number either.or.check + } + if$ +} + +FUNCTION {format.number.series} +{ volume empty$ + { number empty$ + { series field.or.null } + { output.state mid.sentence = + { bbl.number } + { bbl.number capitalize } + if$ + number tie.or.space.connect + series empty$ + { "there's a number but no series in " cite$ * warning$ } + { bbl.in space.word * series * } + if$ + } + if$ + } + { "" } + if$ +} + +FUNCTION {is.num} +{ chr.to.int$ + duplicate$ "0" chr.to.int$ < not + swap$ "9" chr.to.int$ > not and +} + +FUNCTION {extract.num} +{ duplicate$ 't := + "" 's := + { t empty$ not } + { t #1 #1 substring$ + t #2 global.max$ substring$ 't := + duplicate$ is.num + { s swap$ * 's := } + { pop$ "" 't := } + if$ + } + while$ + s empty$ + 'skip$ + { pop$ s } + if$ +} + +FUNCTION {convert.edition} +{ edition extract.num "l" change.case$ 's := + s "first" = s "1" = or + { bbl.first 't := } + { s "second" = s "2" = or + { bbl.second 't := } + { s "third" = s "3" = or + { bbl.third 't := } + { s "fourth" = s "4" = or + { bbl.fourth 't := } + { s "fifth" = s "5" = or + { bbl.fifth 't := } + { s #1 #1 substring$ is.num + { s eng.ord 't := } + { edition 't := } + if$ + } + if$ + } + if$ + } + if$ + } + if$ + } + if$ + t +} + +FUNCTION {format.edition} +{ edition empty$ + { "" } + { output.state mid.sentence = + { convert.edition "l" change.case$ " " * bbl.edition * } + { convert.edition "t" change.case$ " " * bbl.edition * } + if$ + } + if$ +} + +INTEGERS { multiresult } + +FUNCTION {multi.page.check} +{ 't := + #0 'multiresult := + { multiresult not + t empty$ not + and + } + { t #1 #1 substring$ + duplicate$ "-" = + swap$ duplicate$ "," = + swap$ "+" = + or or + { #1 'multiresult := } + { t #2 global.max$ substring$ 't := } + if$ + } + while$ + multiresult +} + +FUNCTION {format.pages} +{ pages empty$ + { "" } + { pages multi.page.check +% { bbl.pages pages n.dashify tie.or.space.connect } +% { bbl.page pages tie.or.space.connect } + { pages n.dashify } + { pages } + if$ + } + if$ +} + +FUNCTION {first.page} +{ 't := + "" + { t empty$ not t #1 #1 substring$ "-" = not and } + { t #1 #1 substring$ * + t #2 global.max$ substring$ 't := + } + while$ +} + +FUNCTION {format.journal.pages} +{ pages empty$ + { format.eprint outputeprint %EDP Sciences le 30/11/2014 + } + { duplicate$ empty$ + { pop$ format.pages } + { + ", " * + pages first.page * + } + if$ + } + if$ +} + +FUNCTION {format.vol.num.pages} +{ volume field.or.null +} + +FUNCTION {format.chapter.pages} +{ chapter empty$ + { "" } + { type empty$ + { bbl.chapter } + { type "l" change.case$ } + if$ + chapter tie.or.space.connect + } + if$ +} + +FUNCTION {format.in.ed.booktitle} +{ booktitle empty$ + { "" } + { editor empty$ + { word.in booktitle emphasize * } + { word.in booktitle emphasize * + ", " * + editor num.names$ #1 > + { bbl.editors } + { bbl.editor } + if$ + * " " * + format.in.editors * + } + if$ + } + if$ +} + +FUNCTION {format.thesis.type} +{ type empty$ + 'skip$ + { pop$ + type "t" change.case$ + } + if$ +} + +FUNCTION {format.tr.number} +{ type empty$ + { bbl.techrep } + 'type + if$ + number empty$ + { "t" change.case$ } + { number tie.or.space.connect } + if$ +} + +FUNCTION {format.article.crossref} +{ + word.in + " \cite{" * crossref * "}" * +} + +FUNCTION {format.book.crossref} +{ volume empty$ + { "empty volume in " cite$ * "'s crossref of " * crossref * warning$ + word.in + } + { bbl.volume volume tie.or.space.connect + bbl.of space.word * + } + if$ + " \cite{" * crossref * "}" * +} + +FUNCTION {format.incoll.inproc.crossref} +{ + word.in + " \cite{" * crossref * "}" * +} + +FUNCTION {format.publisher} +{ publisher empty$ + { "empty publisher in " cite$ * warning$ } + 'skip$ + if$ + "" + address empty$ publisher empty$ and + 'skip$ + { + add.blank "(" * + address empty$ + 'skip$ + { address * } + if$ + publisher empty$ + 'skip$ + { address empty$ + 'skip$ + { ": " * } + if$ + publisher * + } + if$ + ")" * + } + if$ + output +} + +STRINGS {oldname} + +%%%%%%%% To repeat the same authors + +%FUNCTION {name.or.dash} +%{ 's := +% oldname empty$ +% { s 'oldname := s } +% { s oldname = +% { "---" } +% { s 'oldname := s } +% if$ +% } +% if$ +%} + +%%%%%%%% Functions added from astrobib + +FUNCTION {format.edn.btitle} % Title should be on stack. +{ duplicate$ empty$ edition empty$ or + 'skip$ + { ", " * format.edition * } + if$ +} + +FUNCTION {format.ed.booktitle} % The title should be on the stack. +{ duplicate$ empty$ + { "no book title in " cite$ * warning$ "" pop$ } + { editor empty$ + author empty$ or % Empty author means editor already given. + 'format.edn.btitle + { format.edn.btitle ", " * bbl.editor * " " * format.in.editors * } + if$ + } + if$ +} + +FUNCTION {format.full.book.spec} % The title should be on the stack. +{ series empty$ + { format.ed.booktitle + volume empty$ + { number empty$ + 'skip$ + { " there's a number but no series in " cite$ * warning$ + " No." number tie.or.space.connect * } + if$ + } + { ", Vol." volume tie.or.space.connect * + number empty$ + 'skip$ + {"Both volume and number fields in " * cite$ * warning$ } + if$ + } + if$ + } + { volume empty$ + { format.ed.booktitle ", " * series * + number empty$ + 'skip$ + { " No." number tie.or.space.connect * } + if$ + } + { series ", Vol." volume tie.or.space.connect * + ", " * swap$ format.ed.booktitle * + number empty$ + 'skip$ + {"Both volume and number fields in " * cite$ * warning$ } + if$ + } + if$ + } + if$ +} + +%%%%%%% End of functions from astrobib + +FUNCTION {article} +{ output.bibitem + format.authors "author" output.check + author format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block + crossref missing$ + { journal + "journal" output.check + format.vol.num.pages output + } + { format.article.crossref output.nonnull + format.pages output + } + if$ + format.journal.pages + format.note output + %format.eprint outputeprint %EDP Sciences le 30/11/2014 + fin.entry +} + +FUNCTION {book} +{ output.bibitem + author empty$ + { format.editors "author and editor" output.check + editor format.key output +%%%%% name.or.dash + } + { format.authors output.nonnull +%%%%% name.or.dash + crossref missing$ + { "author and editor" editor either.or.check } + 'skip$ + if$ + } + if$ + format.date "year" output.check + date.block + title format.full.book.spec output +% format.btitle "title" output.check +% crossref missing$ +% { format.bvolume output +% format.number.series output +% format.edition output + format.publisher +% } +% { +% format.book.crossref output.nonnull +% } +% if$ + format.pages output + format.note output + fin.entry +} + +FUNCTION {booklet} +{ output.bibitem + format.authors output + author format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block + format.title "title" output.check + howpublished output + address output + format.note output + fin.entry +} + +FUNCTION {inbook} +{ output.bibitem + author empty$ + { format.editors "author and editor" output.check + editor format.key output +%%%%% name.or.dash + } + { format.authors output.nonnull +%%%%% name.or.dash + crossref missing$ + { "author and editor" editor either.or.check } + 'skip$ + if$ + } + if$ + format.date "year" output.check + date.block + title format.full.book.spec output +% format.btitle "title" output.check +% crossref missing$ +% { +% format.bvolume output +% format.chapter.pages "chapter and pages" output.check +% format.number.series output +% format.edition output + format.publisher +% } +% { +% format.chapter.pages "chapter and pages" output.check +% format.book.crossref output.nonnull +% } +% if$ + format.pages "pages" output.check + format.note output + fin.entry +} + +FUNCTION {incollection} +{ output.bibitem + format.authors "author" output.check + author format.key output +%%%%%% name.or.dash + format.date "year" output.check + date.block + bbl.in " " * booktitle format.full.book.spec * output +% crossref missing$ +% { format.in.ed.booktitle "booktitle" output.check +% format.bvolume output +% format.number.series output +% format.edition output +% format.chapter.pages output + format.publisher +% } +% { format.incoll.inproc.crossref output.nonnull +% format.chapter.pages output +% } +% if$ + format.pages "pages" output.check + format.note output + fin.entry +} + +FUNCTION {inproceedings} +{ output.bibitem + format.authors "author" output.check + author format.key output % added + format.date "year" output.check + date.block + bbl.in " " * booktitle format.full.book.spec * output +% crossref missing$ +% { format.in.ed.booktitle "booktitle" output.check +% format.bvolume output +% format.number.series output + publisher empty$ + { organization output + address output + } + { organization output + format.publisher + } + if$ +% } +% { format.incoll.inproc.crossref output.nonnull +% } +% if$ + format.pages output + format.note output + fin.entry +} + +FUNCTION {conference} { inproceedings } + +FUNCTION {manual} +{ output.bibitem + format.authors output + author format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block + format.btitle "title" output.check + format.edition output + organization output + address output + format.note output + fin.entry +} + +FUNCTION {mastersthesis} +{ output.bibitem + format.authors "author" output.check + author format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block +% format.title "title" output.check + bbl.mthesis format.thesis.type output.nonnull + school "school" output.check + address output + format.note output + fin.entry +} + +FUNCTION {misc} +{ output.bibitem + format.authors output + author format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block + format.title output + howpublished output + format.note output + fin.entry +} + +FUNCTION {phdthesis} +{ output.bibitem + format.authors "author" output.check + author format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block +% format.title "title" output.check + bbl.phdthesis format.thesis.type output.nonnull + school "school" output.check + address output + format.note output + fin.entry +} + +FUNCTION {proceedings} +{ output.bibitem + editor empty$ + { organization output + organization format.key output } + { format.editors output } + if$ +% format.editors output +% editor format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block + title format.full.book.spec output +% format.btitle "title" output.check +% format.bvolume output +% format.number.series output + publisher empty$ not % No need for warning if no pub. + { format.publisher } + { editor empty$ % For empty editor, organization was already given. + 'skip$ + { organization output } + if$ + address output + } + if$ +% address output +% organization output +% publisher output + format.pages output + format.note output + fin.entry +} + +FUNCTION {techreport} +{ output.bibitem + format.authors "author" output.check + author format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block + format.title "title" output.check + format.tr.number output.nonnull + institution "institution" output.check + address output + format.note output + fin.entry +} + +FUNCTION {unpublished} +{ output.bibitem + format.authors "author" output.check + author format.key output +%%%%% name.or.dash + format.date "year" output.check + date.block +% format.title "title" output.check + format.note "note" output.check + fin.entry +} + +FUNCTION {default.type} { misc } + +READ + +FUNCTION {sortify} +{ purify$ + "l" change.case$ +} + +INTEGERS { len } + +FUNCTION {chop.word} +{ 's := + 'len := + s #1 len substring$ = + { s len #1 + global.max$ substring$ } + 's + if$ +} + +FUNCTION {format.lab.names} +{ 's := + s #1 "{vv~}{ll}" format.name$ + s num.names$ duplicate$ + #2 > + { pop$ + " {et~al.}" * + } + { #2 < + 'skip$ + { s #2 "{ff }{vv }{ll}{ jj}" format.name$ "others" = + { + " {et~al.}" * + } + { " \& " * s #2 "{vv~}{ll}" format.name$ + * } + if$ + } + if$ + } + if$ +} + +FUNCTION {author.key.label} +{ author empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { author format.lab.names } + if$ +} + +FUNCTION {author.editor.key.label} +{ author empty$ + { editor empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { editor format.lab.names } + if$ + } + { author format.lab.names } + if$ +} + +FUNCTION {editor.key.label} +{ editor empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { editor format.lab.names } + if$ +} + +FUNCTION {calc.short.authors} +{ type$ "book" = + type$ "inbook" = + or + 'author.editor.key.label + { type$ "proceedings" = + 'editor.key.label + 'author.key.label + if$ + } + if$ + 'short.list := +} + +FUNCTION {calc.label} +{ calc.short.authors + short.list + "(" + * + year duplicate$ empty$ + { pop$ "????" } + 'skip$ + if$ + * + 'label := +} + +FUNCTION {sort.format.names} +{ 's := + #1 'nameptr := + "" + s num.names$ 'numnames := + numnames 'namesleft := + { namesleft #0 > } + { s nameptr + "{vv{ } }{ll{ }}{ f{ }}{ jj{ }}" + format.name$ 't := + nameptr #1 > + { + " " * + namesleft #1 = t "others" = and + { "zzzzz" * } + { t sortify * } + if$ + } + { t sortify * } + if$ + nameptr #1 + 'nameptr := + namesleft #1 - 'namesleft := + } + while$ +} + +FUNCTION {sort.format.title} +{ 't := + "A " #2 + "An " #3 + "The " #4 t chop.word + chop.word + chop.word + sortify + #1 global.max$ substring$ +} + +FUNCTION {author.sort} +{ author empty$ + { key empty$ + { "to sort, need author or key in " cite$ * warning$ + "" + } + { key sortify } + if$ + } + { author sort.format.names } + if$ +} + +FUNCTION {author.editor.sort} +{ author empty$ + { editor empty$ + { key empty$ + { "to sort, need author, editor, or key in " cite$ * warning$ + "" + } + { key sortify } + if$ + } + { editor sort.format.names } + if$ + } + { author sort.format.names } + if$ +} + +FUNCTION {editor.sort} +{ editor empty$ + { key empty$ + { "to sort, need editor or key in " cite$ * warning$ + "" + } + { key sortify } + if$ + } + { editor sort.format.names } + if$ +} + +FUNCTION {presort} +{ calc.label + label sortify + " " + * + type$ "book" = + type$ "inbook" = + or + 'author.editor.sort + { type$ "proceedings" = + 'editor.sort + 'author.sort + if$ + } + if$ + #1 entry.max$ substring$ + 'sort.label := + sort.label + * + " " + * + title field.or.null + sort.format.title + * + #1 entry.max$ substring$ + 'sort.key$ := +} + +ITERATE {presort} + +SORT + +STRINGS { last.label next.extra } + +INTEGERS { last.extra.num number.label } + +FUNCTION {initialize.extra.label.stuff} +{ #0 int.to.chr$ 'last.label := + "" 'next.extra := + #0 'last.extra.num := + #0 'number.label := +} + +FUNCTION {forward.pass} +{ last.label label = + { last.extra.num #1 + 'last.extra.num := + last.extra.num int.to.chr$ 'extra.label := + } + { "a" chr.to.int$ 'last.extra.num := + "" 'extra.label := + label 'last.label := + } + if$ + number.label #1 + 'number.label := +} + +FUNCTION {reverse.pass} +{ next.extra "b" = + { "a" 'extra.label := } + 'skip$ + if$ + extra.label 'next.extra := + extra.label + duplicate$ empty$ + 'skip$ + { "{\natexlab{" swap$ * "}}" * } + if$ + 'extra.label := + label extra.label * 'label := +} + +EXECUTE {initialize.extra.label.stuff} + +ITERATE {forward.pass} + +REVERSE {reverse.pass} + +FUNCTION {bib.sort.order} +{ sort.label + " " + * + year field.or.null sortify + * + " " + * + title field.or.null + sort.format.title + * + #1 entry.max$ substring$ + 'sort.key$ := +} + +ITERATE {bib.sort.order} + +SORT + +FUNCTION {begin.bib} +{ preamble$ empty$ + 'skip$ + { preamble$ write$ newline$ } + if$ + "\begin{thebibliography}{" number.label int.to.str$ * "}" * + write$ newline$ + "\expandafter\ifx\csname natexlab\endcsname\relax\def\natexlab#1{#1}\fi" + write$ newline$ +} + +EXECUTE {begin.bib} + +EXECUTE {init.state.consts} + +ITERATE {call.type$} + +FUNCTION {end.bib} +{ newline$ + "\end{thebibliography}" write$ newline$ +} + +EXECUTE {end.bib} +%% End of customized bst file +%% +%% End of file `apj.bst'. + diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa.cls b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa.cls new file mode 100644 index 0000000..ac164cb --- /dev/null +++ b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa.cls @@ -0,0 +1,2068 @@ +%% +%% This is file `aa.cls', +%% generated with the docstrip utility. +%% +%% The original source files were: +%% +%% aa.dtx (with options: `aa') +%% +%% aa.dtx +%% Copyright EDP Sciences, E-press (2016), J.-C. Charpentier (2010), all rights reserved. +%% Class `aa' to use with LaTeX 2e +%% \CharacterTable +%% {Upper-case \A\B\C\D\E\F\G\H\I\J\K\L\M\N\O\P\Q\R\S\T\U\V\W\X\Y\Z +%% Lower-case \a\b\c\d\e\f\g\h\i\j\k\l\m\n\o\p\q\r\s\t\u\v\w\x\y\z +%% Digits \0\1\2\3\4\5\6\7\8\9 +%% Exclamation \! Double quote \" Hash (number) \# +%% Dollar \$ Percent \% Ampersand \& +%% Acute accent \' Left paren \( Right paren \) +%% Asterisk \* Plus \+ Comma \, +%% Minus \- Point \. Solidus \/ +%% Colon \: Semicolon \; Less than \< +%% Equals \= Greater than \> Question mark \? +%% Commercial at \@ Left bracket \[ Backslash \\ +%% Right bracket \] Circumflex \^ Underscore \_ +%% Grave accent \` Left brace \{ Vertical bar \| +%% Right brace \} Tilde \~} +%% +\def\filedate{2016/09/01} +\let\aafiledate\filedate +\def\fileversion{9.1} +\let\aafileversion\fileversion +\NeedsTeXFormat{LaTeX2e}[1995/06/01] +\ProvidesClass{aa} + [\filedate{} v\fileversion{} Class for AA journal] +\LoadClass[fleqn]{article} +\newif\ifaa@letter +\DeclareOption{letter}{\aa@lettertrue} +\newif\ifaa@onlletter +\DeclareOption{onlletter}{\aa@onllettertrue} +\newif\ifaa@online +\DeclareOption{online}{\aa@onlinetrue} +\newif\ifaa@referee +\DeclareOption{referee}{\aa@refereetrue} +\newif\ifaa@contents +\DeclareOption{contents}{\aa@contentstrue} +\newif\ifaa@contentsAut +\DeclareOption{contentsAut}{\aa@contentsAuttrue} +\newlength\aa@fullwidth +\newlength\aa@fullheight +\DeclareOption{a4paper}{% + \renewcommand*\aa@paper{a4paper}% + \setlength\aa@fullwidth{184mm}% + \renewcommand*\aa@leftmarginpaper{(21cm-\aa@fullwidth)/2}% + \setlength\aa@fullheight{705pt}% +} +\DeclareOption{letterpaper}{% + \renewcommand*\aa@paper{letterpaper} + \setlength\aa@fullwidth{184mm}% + \renewcommand*\aa@leftmarginpaper{(8.5in-\aa@fullwidth)/2}% + \setlength\aa@fullheight{705pt-1.76cm}% +} +\DeclareOption{legalpaper}{% + \renewcommand*\aa@paper{legalpaper}% + \setlength\aa@fullwidth{184mm}% + \renewcommand*\aa@leftmarginpaper{(8.5in-\aa@fullwidth)/2}% + \setlength\aa@fullheight{705pt}% +} +\newcommand*\aa@paper{} +\newcommand*\aa@leftmarginpaper{} +\newif\ifaa@twocolumn +\DeclareOption{onecolumn}{% + \aa@twocolumnfalse + \renewcommand*\aa@column{onecolumn}% +} +\DeclareOption{twocolumn}{% + \aa@twocolumntrue + \renewcommand*\aa@column{twocolumn}% +} +\newcommand*\aa@column{} +\newif\if@wideboxfn +\@wideboxfnfalse +\DeclareOption{wideboxfn}{\@wideboxfntrue} +% +\newif\ifaa@longfn +\DeclareOption{longfn}{\aa@longfntrue} +\newif\ifaa@longauth +\DeclareOption{longauth}{\aa@longauthtrue} +\let\if@myobjects\iffalse +\DeclareOption{ascii}{% + \def\aa@inputenc{\RequirePackage[ascii]{inputenc}}% +} +\DeclareOption{latin1}{% + \def\aa@inputenc{\RequirePackage[latin1]{inputenc}}% +} +\DeclareOption{latin9}{% + \def\aa@inputenc{\RequirePackage[latin9]{inputenc}}% +} +\DeclareOption{ansinews}{% + \def\aa@inputenc{\RequirePackage[ansinews]{inputenc}}% +} +\DeclareOption{applemac}{% + \def\aa@inputenc{\RequirePackage[applemac]{inputenc}}% +} +\DeclareOption{utf8}{% + \def\aa@inputenc{\RequirePackage[utf8]{inputenc}}% +} +\newcommand*\aa@font{} +\DeclareOption{cm}{% + \def\aa@font{% + \RequirePackage{textcomp}% + }% +} +\DeclareOption{showoverfull}{\setlength\overfullrule{5\p@}} +\DeclareOption{hideoverfull}{\setlength\overfullrule{\z@}} +\DeclareOption{openbib}{% + \AtEndOfPackage{% + \renewcommand\@openbib@code{% + \advance\leftmargin\bibindent + \itemindent -\bibindent + \listparindent \itemindent + \parsep \z@ + }% + \renewcommand\newblock{\par}}% +} +\newif\ifaa@bibnumber +\DeclareOption{bibnumber}{\aa@bibnumbertrue% + \def\aa@biblio{% + \RequirePackage[sort&compress]{natbib} + \bibpunct{[}{]}{,}{n}{}{,}% + \def\@biblabel##1{##1.}% + \bibliographystyle{plainnat}% + \def\bibfont{\aa@bibliographyfont}% + \setlength{\bibsep}{\z@}% + } +} +\DeclareOption{bibauthoryear}{% + \def\aa@biblio{% + \RequirePackage{natbib} + \bibpunct{(}{)}{;}{a}{}{,}% + \def\bibfont{\aa@bibliographyfont}% + \setlength{\bibsep}{\z@}% + }% +} +\DeclareOption{bibyear}{% + \def\aa@biblio{% + \def\@biblabel##1{}% + \def\@cite##1##2{{##1\if@tempswa , ##2\fi}}% + } +} +\ExecuteOptions{a4paper,twocolumn,utf8,hideoverfull,bibauthoryear} +\ProcessOptions +\RequirePackage{calc} +\RequirePackage{etex} +\RequirePackage[T1]{fontenc} +\aa@inputenc +\aa@font +\ifaa@referee +\RequirePackage{xcolor} +\RequirePackage{marginnote} +\AtEndOfClass{ +\setlength{\marginparwidth}{50mm} +\setlength{\marginparsep}{5mm} +} +% +\newcounter{lenote} +\AtBeginDocument{% +\@ifpackageloaded{hyperref}% +{\newcommand{\LEm}[1]{\texorpdfstring{\protect\stepcounter{lenote}{\normalfont\textbf{\color{red}[Note \arabic{lenote}] }} +\protect\marginnote{\baselineskip3ex{\normalsize{\normalfont\textbf{\color{red}[Note \arabic{lenote}: #1]}}}}}{}} +\newcommand{\LEt}[1]{\texorpdfstring{\protect\stepcounter{lenote}\normalfont\textbf{\color{red}[Note \arabic{lenote}: #1] }}{}}}% +{\newcommand{\LEm}[1]{\protect\stepcounter{lenote}{\normalfont\textbf{\color{red}[Note \arabic{lenote}] }} +\protect\marginnote{\baselineskip3ex{\normalsize{\normalfont\textbf{\color{red}[Note \arabic{lenote}: #1]}}}}} +\newcommand{\LEt}[1]{\protect\stepcounter{lenote}\normalfont\textbf{\color{red}[Note \arabic{lenote}: #1] }}}% +} + \renewcommand*\aa@column{onecolumn} + \aa@twocolumnfalse + \setlength{\aa@fullwidth}{0.75\aa@fullwidth} + \renewcommand*\aa@leftmarginpaper{15mm} + \if!\csname 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#1{{\aa@longtableheadcaptionfont#2.} }#3% + }% + \ifdim\wd\@tempboxa>\hsize + #1{{\aa@longtableheadcaptionfont#2.} }#3% + \else + \hbox to\hsize{\box\@tempboxa\hfil}% + \fi + \endgraf\vskip\baselineskip + }% + \hss + }% + }% +} +\aa@biblio +\RequirePackage{xspace} +\RequirePackage[english]{babel} +\def\aatolm#1{\gdef\@aatolm{#1}} +\def\@aatolm{} +\renewenvironment{appendix}{\par\clearpage\aatolm{1} +\def\@hangfrom##1{\setbox\@tempboxa\hbox{{##1}}% + \hangindent \parindent\noindent\box\@tempboxa} +\def\sectcounterend{:} +\def\@seccntformat##1{\appendixname\ \csname the##1\endcsname\sectcounterend% + \hskip\betweenumberspace} + \setcounter{section}{0}% + \setcounter{subsection}{0}% + \setcounter{figure}{0}% + \setcounter{table}{0}% + \renewcommand\thesection{\@Alph\c@section}% + \renewcommand\thesubsection{\@Alph\c@section.\@arabic\c@subsection}% + \renewcommand\thesubsubsection{\thesubsection.\@arabic\c@subsubsection}% + \renewcommand\theequation{\@Alph\c@section.\@arabic\c@equation}% + 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+\newcommand*\aa@contentsname{Contents sorted by section} +\newcommand*\aa@contentsAutname{Contents sorted by first author} +\newcommand*\aa@pagename{page} +\newcommand*\aa@AAname{A\&A} +\newcommand*\aa@copyrightname{\copyright~ESO} +\newcommand*\aa@subabstractiname{Context} +\newcommand*\aa@subabstractiiname{Aims} +\newcommand*\aa@subabstractiiiname{Methods} +\newcommand*\aa@subabstractivname{Results} +\newcommand*\aa@subabstractvname{Conclusions} +\newcommand*\aa@keywordname{Key words} +\newcommand*\aa@acknowledgementsname{Acknowledgements} +\newcommand*\aa@floatcounterend{.~} +\newcommand*\aa@tablebibname{References} +\newcommand*\aa@tablefootname{Notes} +\renewcommand\normalsize{% + \@setfontsize\normalsize\@xpt{11}% + \abovedisplayskip 8.55\p@ \@plus4\p@ \@minus5\p@ + \abovedisplayshortskip \z@ \@plus3\p@ + \belowdisplayshortskip 6\p@ \@plus3\p@ \@minus3\p@ + \belowdisplayskip \abovedisplayskip + \let\@listi\@listI} +\normalsize +\renewcommand\small{% + 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+\newcommand*\aa@logo@astronomyfont{\fontsize{18}{21}\sffamily\bfseries} +\newcommand*\aa@logo@andfont{\fontsize{16}{12}\sffamily\mdseries} +\newcommand*\aa@logo@astrophysicsfont{\fontsize{18}{21}\sffamily\bfseries} +\newcommand*\aa@letternamefont{\sffamily\fontsize{19.2\p@}{21\p@}\bfseries} +\newcommand*\aa@headletternamefont{\large\scshape} +\newcommand*\aa@contentsnamefont{\Large\sffamily\bfseries} +\newcommand*\aa@contentsAutnamefont{\Large\sffamily\bfseries} +\newcommand*\aa@journalnamefont{\slshape} +\newcommand*\aa@manuscriptnamefont{} +\newcommand*\aa@todayheadboxfont{} +\newcommand*\aa@msnrheadboxfont{\LARGE\bfseries\smash} +\newcommand*\aa@textidlineempty{{\slshape A\&A proofs:}\ manuscript no.~\jobname} +\newcommand*\aa@idlinefont{} +\newcommand*\aa@doifont{} +\newcommand*\aa@copyrightfont{\small} +\ifaa@letter + \definecolor{aa@colorletter}{gray}{0.6} +\fi +\newcommand*\aa@topicsfont{\fontsize{12}{14}\sffamily\itshape} +\newcommand*\aa@topicsnamefont{\fontsize{17}{20}\sffamily} +\newcommand*\aa@headnotefont{\LARGE\itshape} +\newcommand*\aa@defaultheadnotefont{\LARGE\sffamily\bfseries\itshape} +\newcommand*\aa@titlefont{\LARGE \sffamily\bfseries\boldmath} +\newcommand*\aa@subtitlefont{\Large \sffamily\bfseries\boldmath} +\newcommand*\aa@authorfont{\large} +\newcommand*\aa@institutefont{\small} +\newcommand*\aa@datefont{\small} +\newcommand*\aa@dedicationfont{\itshape} +\newcommand*\aa@abstractnamefont{\small\sffamily\bfseries\MakeUppercase} +\newcommand*\aa@keywordnamefont{\small\sffamily\bfseries} +\newcommand*\aa@keywordfont{\small} +\newcommand*\aa@longauthfont{\centering\small\itshape} +\newcommand*\aa@longauthname{Affiliations can be found after the references} +\newcommand*\aa@longauthopen{(} +\newcommand*\aa@longauthclose{)} +\newcommand*\aa@acknowledgementsfont{\tiny} +\newcommand*\aa@acknowledgementsnamefont{\itshape} +\newcommand*\aa@bibliographyfont{\tiny} +\newcommand*\aa@captionfont{\normalfont\small} +\newcommand*\aa@headcaptionfont{\bfseries} +\newcommand*\aa@tablebibfont{\small} +\newcommand*\aa@tablebibnamefont{\small\bfseries} +\newcommand*\aa@tablefootfont{\small} +\newcommand*\aa@tablefootnamefont{\small\bfseries} +\newcommand*\aa@descriptionlabelfont{} +\newcommand\aa@longtablecaptionfont{\small} +\newcommand\aa@longtableheadcaptionfont{\small\bfseries} +\newcommand*\aa@emailfont{\ttfamily} +\newcommand*\aa@entryifont{\itshape} +\newcommand*\aa@entryiifont{\bfseries} +\newtoks\authorlink +\newtoks\yearCop +\newbox\aa@stripbox +\newbox\aa@outputbox +\newenvironment{aa@strip} +{% + \onecolumn\parindent0mm + \setbox\aa@stripbox=\vbox\bgroup +} +{% + \egroup + \aa@@strip +} +\def\aa@@strip{% + \ifdim\ht\aa@stripbox>\textheight + \global\setbox\aa@outputbox=\vsplit\aa@stripbox to \textheight + \dp\aa@outputbox \z@ + \box\aa@outputbox\clearpage + \expandafter\aa@@strip + \else + \dp\aa@stripbox \z@ + \twocolumn[\box\aa@stripbox] + \fi +} +\newcommand{\ErratumOf}[3][]{} +\newcommand{\NoteFor}[3][]{} +\renewcommand*\@fnsymbol[1]{% + \ensuremath{% + \ifcase#1 + \or\star + \or{\star}{\star} + \or{\star}{\star}{\star}% + \or{\star}{\star}{\star}{\star} + \or \dagger + \or \ddagger + \or \mathsection + \or \mathparagraph + \or \| + \or ** + \or \dagger\dagger + \or \ddagger\ddagger + \else \@ctrerr + \fi + }% +} +\newcommand\longempty{} +\newcommand*\aa@cntwords[1]{% + \protected@edef\aa@cntwords@arg{#1\space\noexpand\aa@nil\space}% + \aa@nbwords \z@ + \let\@@protect\protect + \let\protect\@unexpandable@protect + \expandafter\aa@@cntwords\aa@cntwords@arg + \restore@protect +} +\newcommand*\aa@nnil{\aa@nil} +\long\def\aa@@cntwords#1 {% + \def\aa@arg{#1}% + \ifx\aa@arg\aa@nnil + \else + \advance\aa@nbwords \@ne + \expandafter\aa@@cntwords + \fi +} +\newcommand*\aa@roheadletter{% + \setlength{\aa@dima} + {1in + \topmargin + \headheight - \dp\strutbox + + 2\aa@bleedmargin}% + \setlength{\aa@dimb} + {\paperwidth - (1in + \oddsidemargin + \textwidth) + + \aa@bleedmargin - \aa@hoffsetgray}% + \setbox0=\hbox{\aa@letternamefont \lettername}% + \setlength{\aa@dimc} + {\paperheight - \aa@dima - \wd0 + 2\aa@bleedmargin}% + \addtolength{\aa@voffsetlettername}{0.5cm} + \leavevmode + \hbox to0pt{% + \hspace*{\aa@hoffsetgray}% + \vbox to0pt{% + \hsize=\aa@dimb + \vskip-\aa@dima + \colorbox{aa@colorletter}{% + \vtop{% + \vspace*{\aa@voffsetlettername}% + \hspace*{\aa@hoffsetlettername}% + \rotatebox{90}{\aa@letternamefont \lettername}% + \hfill\null + \vspace*{\aa@dimc}% + }% + }% + \vss + }% + \hss + }% +} +\newcommand*\aa@leheadletter{% + \setlength{\aa@dima} + {1in + \topmargin + \headheight - \dp\strutbox + + 2\aa@bleedmargin}% + \setlength{\aa@dimb} + {1in + \oddsidemargin + \aa@bleedmargin - \aa@hoffsetgray}% + \setbox0=\hbox{\aa@letternamefont \lettername}% + \setlength{\aa@dimc} + {\paperheight-\aa@dima-\wd0+2\aa@bleedmargin}% + \addtolength{\aa@voffsetlettername}{0.5cm} + \leavevmode + \hspace*{-2\fboxsep}% + \hbox to0pt{% + \hss + \vbox to0pt{% + \hsize=\aa@dimb + \vskip-\aa@dima + \colorbox{aa@colorletter}{% + \vtop{% + \vspace*{\aa@voffsetlettername}% + \hfill + \rotatebox{90}{\aa@letternamefont \lettername}% + \hspace*{\aa@hoffsetlettername}% + \vspace*{\aa@dimc}% + }% + }% + \vss + }% + \hspace*{\aa@hoffsetgray}% + }% +} +\ifaa@online + \fancypagestyle{firstpage}{% + \fancyhf{}% + \renewcommand*{\headrulewidth}{\z@}% + \renewcommand*{\footrulewidth}{\z@}% + \fancyfoot[RO]{\aa@footfont\aa@publishlink\aa@numarticle\aa@pageof}% + \fancyfoot[LE]{\aa@footfont\aa@numarticle\aa@pageof\qquad\aa@publishlink}% + } +\else + \fancypagestyle{firstpage}{% + \fancyhf{}% + \renewcommand*{\headrulewidth}{\z@}% + \renewcommand*{\footrulewidth}{\z@}% + \fancyfoot[RO]{\aa@footfont \aa@numarticle\aa@pageof}% + \fancyfoot[LE]{\aa@footfont \aa@numarticle\aa@pageof}% + } +\fi +\ifaa@contents + \fancypagestyle{otherpage}{% + \fancyhf{}% + \fancyhead[C]{\aa@AAname}% + \fancyfoot[C]{\aa@contentsname, \aa@pagename\space \thepage}% + \renewcommand*{\headrulewidth}{\z@}% + \renewcommand*{\footrulewidth}{\z@}% + } +\else\ifaa@contentsAut + \fancypagestyle{otherpage}{% + \fancyhf{}% + \fancyhead[C]{\aa@AAname}% + \fancyfoot[C]{\aa@contentsAutname, \aa@pagename\space \thepage}% + \renewcommand*{\headrulewidth}{\z@}% + \renewcommand*{\footrulewidth}{\z@}% + } +\else + \fancypagestyle{otherpage}{% + \fancyhf{}% + \fancyhead[CO]{\aa@headfont \aa@headings}% + \fancyhead[CE]{\aa@headfont \ifx\aa@idline\empty\aa@textidlineempty\else\aa@idline\fi}% + \fancyfoot[RO]{\aa@footfont \aa@numarticle\aa@pageof}% + \fancyfoot[LE]{\aa@footfont \aa@numarticle\aa@pageof}% + \renewcommand*{\headrulewidth}{\z@}% + \renewcommand*{\footrulewidth}{\z@}% + } +\fi\fi +\pagestyle{otherpage} +\newcommand*\aa@headings{} +\renewcommand*\date[1]{\renewcommand*\aa@date{#1}}% +\newcommand*\aa@date{\today} +\renewcommand*\title[1]{\renewcommand*\aa@title{#1}}% +\newcommand*\aa@title{} +\newcommand*\subtitle[1]{\renewcommand*\aa@subtitle{#1}} +\newcommand*\aa@subtitle{} +\renewcommand*\author[1]{% + \renewcommand*\aa@author{#1}% + \begingroup + \let\and\relax + \renewcommand*\inst[1]{}% + \renewcommand*\thanks[1]{}% + \renewcommand*\email[1]{}% + \let\@@protect\protect + \let\protect\@unexpandable@protect + \global\aa@nbauthors \z@ + \expandafter\aa@cntauthors\aa@author\and\aa@nil\and + \restore@protect + \endgroup +}% +\newcommand*\aa@author{} +\def\aa@cntauthors#1\and{% + \def\aa@arg{#1}% + \ifx\aa@arg\aa@nnil + \else + \global\advance\aa@nbauthors \@ne + \expandafter\aa@cntauthors + \fi +} +\newcommand*\institute[1]{% + \renewcommand*\aa@institute{#1} + \begingroup + \let\and\relax + \renewcommand*\inst[1]{}% + \renewcommand*\thanks[1]{}% + \renewcommand*\email[1]{}% + \let\@@protect\protect + \let\protect\@unexpandable@protect + \global\aa@nbinstitutes \z@ + \expandafter\aa@cntinstitutes\aa@institute\and\aa@nil\and + \restore@protect + \endgroup +}% +\newcommand*\aa@institute{} +\def\aa@cntinstitutes#1\and{% + \def\aa@arg{#1}% + \ifx\aa@arg\aa@nnil + \else + \global\advance\aa@nbinstitutes \@ne + \expandafter\aa@cntinstitutes + \fi +} +\newcommand*\inst[1]{\unskip\hbox{\@textsuperscript{\normalfont$#1$}}} +\newcommand*\fnmsep{\unskip\hbox{\@textsuperscript{\normalfont,}}} +\newcommand*\email[1]{e-mail: {\aa@emailfont #1}} +\let\endabstract\relax +\renewcommand\abstract[1]{% + \renewcommand\aa@abstract@i{#1}% + \@ifnextchar\bgroup{\aa@abstract@next}{\aa@abstract@one} +} +\newcommand\aa@abstract@next[4]{% + \aa@structabstracttrue + \renewcommand\aa@abstract@ii{#1}% + \renewcommand\aa@abstract@iii{#2}% + \renewcommand\aa@abstract@iv{#3}% + \renewcommand\aa@abstract@v{#4}% + \begingroup + \renewcommand\thanks[1]{}% + \protected@xdef\aa@abstractwords{% + \aa@abstract@i \space + \aa@abstract@ii \space + \aa@abstract@iii \space + \aa@abstract@iv \space + \aa@abstract@v \space + }% + \endgroup + \aa@cnta \z@ + \aa@cntb \aa@structabstractmax + \aa@abstract@cnt +} +\newcommand*\aa@abstract@one{% + \protected@xdef\aa@abstractwords{\aa@abstract@i}% + \aa@cnta \z@ + \aa@cntb \aa@traditabstractmax + \aa@abstract@cnt +} +\def\aa@abstract@cnt{% + \aa@cntwords\aa@abstractwords + \advance\aa@nbwords \aa@cnta\relax + \ifnum\aa@nbwords>\aa@cntb + \typeout{^^J^^JIMPORTANT} + \ClassWarning{aa} + {Around \the\aa@nbwords\space words in the abstract instead + of \the\aa@cntb\space (max). You should rewrite your abstract} + \typeout{IMPORTANT + ^^J} + \fi +} +\newcommand\aa@abstract@i{} +\newcommand\aa@abstract@ii{} +\newcommand\aa@abstract@iii{} +\newcommand\aa@abstract@iv{} +\newcommand\aa@abstract@v{} +\newcommand*\keywords[1]{% + \renewcommand*\aa@keywords{#1}% + \aa@keywords@cnt + \ifnum\aa@nbwords>\aa@keywordsmax + \ClassWarning{aa} + {\the\aa@nbwords\space keywords instead of a maximum of + \aa@keywordsmax\space} + \fi +} +\newcommand*\aa@keywords{} +\newcommand*\aa@doublehyphen{--} +\newcommand*\aa@keywords@cnt{% + \protected@edef\aa@@keywords{\aa@keywords--\noexpand\aa@nil--}% + \aa@nbwords \z@ + \let\@@protect\protect + \let\protect\@unexpandable@protect + \expandafter\aa@@keywords@cnt\aa@@keywords + \restore@protect +} +\def\aa@@keywords@cnt#1--{% + \def\aa@arg{#1}% + \ifx\aa@arg\aa@nnil + \else + \advance\aa@nbwords \@ne + \expandafter\aa@@keywords@cnt + \fi +} +\newcommand*\topics[1]{\renewcommand*\aa@topics{#1}} +\newcommand*\aa@topics{} +\newcommand*\titlerunning[1]{% + \renewcommand*\aa@titlerunning{#1} +} +\newcommand*\aa@titlerunning{} +\newcommand*\authorrunning[1]{% + \renewcommand*\aa@authorrunning{#1} +} +\newcommand*\aa@authorrunning{} +\newcommand*\offprints[1]{% + \protected@edef\@thanks{% + \@thanks + \protect\footnotetext[0]{% + \unskip% + \if@wideboxfn% + \hspace{\aa@removefootnotewbindentspace}% + \else% + \hspace{\aa@removefootnoteindentspace}% + \fi + {% + \aa@offprintsnamefont + \aa@offprintsname + }: \ignorespaces#1% + }% + }% +} +\def\aainstitutename{\par + \begingroup + \renewcommand*\and{% + \par\refstepcounter{aa@institutecnt}% + \hangindent\aa@instituteindent + \noindent + \hbox to\aa@instituteindent{% + \hss + \hbox{\@textsuperscript{\normalfont\theaa@institutecnt}}% + \enspace + }% + \ignorespaces + }% + \ifnum\aa@nbinstitutes>99 + \setbox0=\hbox{\hbox{\@textsuperscript{\normalfont888}}\enspace}% + \else\ifnum\aa@nbinstitutes>9 + \setbox0=\hbox{\hbox{\@textsuperscript{\normalfont88}}\enspace}% + \else + \setbox0=\hbox{\hbox{\@textsuperscript{\normalfont8}}\enspace}% + \fi\fi + \aa@instituteindent \wd0 + {% + \aa@institutefont + \par\refstepcounter{aa@institutecnt}% + \ifnum\aa@nbinstitutes=1\relax + \noindent\ignorespaces + \else + \hangindent\aa@instituteindent + \noindent + \hbox to\aa@instituteindent{% + \hss + \hbox{\@textsuperscript{\normalfont\theaa@institutecnt}}% + \enspace + }\ignorespaces% + \fi% + \aa@institute\par + } + \endgroup} +\newcommand*\mail[1]{\renewcommand*\aa@mail{#1}} +\newcommand*\aa@mail{} +\newcommand*\msnr[1]{\renewcommand*\aa@msnr{#1}} +\newcommand*\aa@msnr{} +\newcommand*\idline[1]{\renewcommand*\aa@idline{#1}} +\newcommand*\aa@idline{} +\newcommand*\headnote[1]{\renewcommand*\aa@headnote{#1}} +\newcommand*\aa@headnote{} +\newcommand*\aa@defaultheadnote{Corrigendum} +\newcommand*\dedication[1]{\renewcommand*\aa@dedication{#1}} +\newcommand*\aa@dedication{} +\renewcommand*\maketitle{% + \thispagestyle{firstpage} +\begingroup + \if@wideboxfn + \setlength\bibindent{1.4\parindent} + \else + \setlength\bibindent{\parindent} + \fi + \renewcommand*\thefootnote{\@fnsymbol\c@footnote}% + \renewcommand\@makefntext[1]{% + \ifaa@longfn\hsize\textwidth\fi + \noindent + \hb@xt@\bibindent{\hss\@makefnmark\enspace}##1} + \ifaa@twocolumn + \begingroup + \twocolumn[\aa@maketitle] + \@thanks + \endgroup + \else + \begingroup + \let\thanks\footnote + \aa@maketitle + \endgroup + \fi +\endgroup + \setcounter{footnote}{0}% +} +\newcommand*\aa@maketitle{% + \ifaa@contents + {\aa@contentsnamefont \aa@contentsname\par} + \addvspace{\aa@aftercontentsnameskip} + \else\ifaa@contentsAut + {\aa@contentsAutnamefont \aa@contentsAutname\par} + \addvspace{\aa@aftercontentsAutnameskip} + \else + \vbox to0pt{\vskip\aa@beforeheadboxskip + \nointerlineskip + \ifx\aa@idline\empty + \noindent + \fbox{% + \begin{minipage}{\linewidth-2\fboxsep-2\fboxrule} + \strut + {\aa@journalnamefont \aa@journalname} + {\aa@manuscriptnamefont \aa@manuscriptname}\\ + \ifx\aa@msnr\empty + {\strut\aa@todayheadboxfont \today}% + \else + \makebox[0.75\linewidth][r]{% + \strut + {\aa@msnrheadboxfont \aa@msnr}% + }% + \fi + \end{minipage}% + }% + \else + \begin{tabular}[b]{@{}l@{}} + \aa@idlinefont \aa@idline\\ + \aa@doifont \aa@doi\\ + \aa@copyrightfont \aa@copyrightname~\if!\the\yearCop!\the\year\else\the\yearCop\fi + \end{tabular} + \hfill\AALogo + \fi\vss} + \par + \ifx\aa@topics\empty% + \addvspace{\aa@afterheadboxskip} + \else + \addvspace{\aa@beforetopicsskip} + {\noindent\aa@topicsfont \aa@topics}% + \hfill + {\aa@topicsnamefont \aa@topicsname\par} + \addvspace{\aa@aftertopicsskip} + \fi + \begingroup + \centering + \ifaa@letter + \ifx\aa@topics\empty + \addvspace{1.8\aa@beforeletternameskip} + \else + \addvspace{\aa@beforeletternameskip} + \fi + {\aa@headletternamefont \lettername\par} + \addvspace{\aa@afterletternameskip} + \fi + \ifx\aa@headnote\empty\else + \ifx\aa@headnote\aa@defaultheadnote\else + {\aa@headnotefont \aa@headnote\par} + \addvspace{\aa@afterheadnoteskip} + \fi + \fi + {\aa@titlefont \aa@title\par} + \ifx\aa@subtitle\empty% + \ifx\aa@headnote\aa@defaultheadnote + {\aa@defaultheadnotefont (\aa@headnote)\par} + \fi + \addvspace{\aa@aftertitleskip} + \else + \addvspace{\aa@aftertitleskip} + {\aa@subtitlefont \aa@subtitle\par} + \ifx\aa@headnote\aa@defaultheadnote + \addvspace{\aa@beforedefaultheadnoteskip} + {\aa@defaultheadnotefont (\aa@headnote)\par} + \fi + \addvspace{\aa@aftersubtitleskip} + \fi + \ifnum\aa@nbauthors=\tw@ + \let\and\andtwoname + \else + \renewcommand\and{% + \advance\aa@cnta \@ne + \ifnum\aa@cnta=\aa@nbauthors + \andlastname + \else + \andname + \fi + } + \fi + \aa@cnta \@ne + {\aa@authorfont \aa@author\par} + \addvspace{\aa@afterauthorskip} + \endgroup + \begingroup + \ifaa@longauth\addvspace{-10pt} + {\noindent\aa@longauthfont% + \aa@longauthopen\aa@longauthname\aa@longauthclose\par} + \else + \leftskip \aa@headingleftmargin + \rightskip \aa@headingrightmargin + \aainstitutename + \fi + \vspace{\aa@afterinstituteskip} + {\noindent\aa@datefont\ifaa@longauth\centering\fi \aa@date\par} + \ifx\aa@dedication\empty + \vspace{\aa@afterdateskip} + \else + \addvspace\baselineskip + {\noindent\aa@dedicationfont \aa@dedication\par} + \vspace{\aa@afterdedicationskip} + \fi + {\centering\aa@abstractnamefont \abstractname\par} + \vspace{\aa@afterabstractnameskip} + \ifaa@structabstract + \ifx\aa@abstract@i\longempty\else + {\noindent\aa@subabstractfont \aa@subabstractiname. }% + {\aa@abstractfont \ignorespaces\aa@abstract@i\par} + \vspace{\aa@aftersubabstractskip} + \fi + {\noindent\aa@subabstractfont \aa@subabstractiiname. }% + {\aa@abstractfont \ignorespaces\aa@abstract@ii\par} + \vspace{\aa@aftersubabstractskip} + {\noindent\aa@subabstractfont \aa@subabstractiiiname. }% + {\aa@abstractfont \ignorespaces\aa@abstract@iii\par} + \vspace{\aa@aftersubabstractskip} + {\noindent\aa@subabstractfont \aa@subabstractivname. }% + {\aa@abstractfont \ignorespaces\aa@abstract@iv\par} + \vspace{\aa@aftersubabstractskip} + \ifx\aa@abstract@v\longempty\else + {\noindent\aa@subabstractfont \aa@subabstractvname. }% + {\aa@abstractfont \ignorespaces\aa@abstract@v\par} + \fi + \else + {\noindent\aa@abstractfont \ignorespaces\aa@abstract@i\par} + \fi + \vspace{\aa@afterabstractskip} + \ifx\aa@keywords\empty\else + \noindent + {\aa@keywordnamefont \aa@keywordname. } + {\aa@keywordfont \ignorespaces\aa@keywords\par} + \vspace{\aa@afterkeywordsskip} + \fi + \endgroup + \renewcommand*\thanks[1]{}% + \renewcommand*\inst[1]{}% + \renewcommand*\fnmsep{}% + \renewcommand*\and{, }% + \renewcommand*\\{ }% + \renewcommand*\vspace[1]{}% + \renewcommand*\offprints[1]{}% + \protected@xdef\aa@PDFauthor{\if!\the\authorlink!\aa@author\else\the\authorlink\fi}% + \protected@xdef\aa@PDFtitle{\noexpand\protect\noexpand\aa@title}% + \def\object##1{##1}% + \ifx\aa@authorrunning\empty + \let\and\relax + \renewcommand*\\{\unskip\space\ignorespaces}% + \ifnum\aa@nbauthors=1 + \expandafter\aa@extractoneauthor\aa@author\and\aa@nil + \else\ifnum\aa@nbauthors=2 + \expandafter\aa@extracttwoauthor\aa@author\and\aa@nil + \else + \expandafter\aa@extractoneauthor\aa@author\and\aa@nil + \protected@xdef\aa@headings{\aa@headings\unskip\space\etalname\space}% + \fi\fi + \else + \xdef\aa@headings{\aa@authorrunning}% + \fi + \ifx\aa@titlerunning\empty + \protected@xdef\aa@headings{\aa@headings\unskip: \aa@title}% + \else + \protected@xdef\aa@headings{\aa@headings\unskip: \aa@titlerunning}% + \fi + \setbox0=\hbox{% + \hspace*{\aa@securityheadmargin}% + \aa@headfont \aa@headings + }% + \ifdim\wd0>\aa@fullwidth + \typeout{^^J^^JIMPORTANT} + \ClassWarning{aa} + {The running head built automatically + from \string\author\space and \string\title + exceeds the pagewidth, please supply a shorter form + with \string\authorrunning\space and/or + \string\titlerunning\space prior to \string\maketitle} + {Use \string\titlerunning\space to supply a shorter + title and/or \string\authorrunning\space to supply a + shorter list of authors.}% + \typeout{IMPORTANT + ^^J} + \fi + \fi\fi +} +\def\aa@extractoneauthor#1\and#2\aa@nil{% + \gdef\aa@headings{#1}% +} +\def\aa@extracttwoauthor#1\and#2\and#3\aa@nil{% + \gdef\aa@headings{#1\andtwoname#2}% +} +\def\sectcounterend{.} +\def\@seccntformat#1{\csname the#1\endcsname\sectcounterend +\hskip\betweenumberspace} +\def\@sect#1#2#3#4#5#6[#7]#8{% + \ifnum #2>\c@secnumdepth + \let\@svsec\@empty + \else + \refstepcounter{#1}% + \protected@edef\@svsec{\@seccntformat{#1}\relax}% + \fi + \@tempskipa #5\relax + \ifdim \@tempskipa>\z@ + \begingroup + #6{% + \@hangfrom{\hskip #3\relax\@svsec}% + \raggedright + \hyphenpenalty \@M% + \interlinepenalty \@M #8\@@par}% + \endgroup + \csname #1mark\endcsname{#7}% + \addcontentsline{toc}{#1}{% + \ifnum #2>\c@secnumdepth \else + \protect\numberline{\csname the#1\endcsname}% + \fi + #7}% + \else + \def\@svsechd{% + #6{\hskip #3\relax + \@svsec #8\hskip\aftertext}% + \csname #1mark\endcsname{#7}% + \addcontentsline{toc}{#1}{% + \ifnum #2>\c@secnumdepth \else + \protect\numberline{\csname the#1\endcsname}% + \fi + #7}}% + \fi + \@xsect{#5}} +\ifaa@contentsAut + \renewcommand\section{% + \@startsection{section} + {1} + {\z@} + {-16dd \@plus-4\p@ \@minus-4\p@} + {6dd} + {\large\bfseries\boldmath\MakeUppercase}% + } +\else\ifaa@contents + \renewcommand\section{% + \@startsection{section} + {1} + {\z@} + {-16dd \@plus-4\p@ \@minus-4\p@} + {6dd} + {\large\bfseries\boldmath\MakeUppercase}% + } +\else + \renewcommand\section{% + \@startsection{section} + {1} + {\z@} + {-16dd\@plus-4\p@ \@minus-4\p@} + {6dd} + {\large\sffamily\bfseries\boldmath}% + } +\fi\fi +\renewcommand\subsection{% + \@startsection{subsection} + {2} + {\z@} + {-16dd} + {6dd} + {\normalsize\sffamily\itshape}% +} +\renewcommand\subsubsection{% + \@startsection{subsubsection} + {3} + {\z@} + {-16dd} + {6dd} + {\normalsize\sffamily}% +} +\renewcommand\paragraph{% + \@startsection{paragraph} + {4} + {\z@} + {-16dd} + {-\fontdimen2\font + \@plus-\fontdimen3\font + \@minus-\fontdimen4\font} + {\normalsize\sffamily}% +} +\renewcommand\subparagraph{% + \ClassError{aa}{Command \string\subparagrap\space isn't allowed} + {Only commands from \string\section\space to + \string\paragraph\space are allowed.} +} +\renewcommand\part{% + \ClassError{aa}{Command \string\part\space isn't allowed} + {Only commands from \string\section\space to + \string\paragraph\space are allowed.} +} +\frenchspacing +\clubpenalty=10000 +\widowpenalty=10000 +\flushbottom +\ifaa@twocolumn + \sloppy +\fi +\newenvironment{nopar} + {\let\par\relax% + \aa@acknowledgementsfont + {% + \noindent\aa@acknowledgementsnamefont + \aa@acknowledgementsname.% + }% + \hskip.5em + }{} +\newenvironment{acknowledgements} + {% + \par\addvspace{\aa@beforeacknowledgementsskip} + \begin{spacing}{0.81} + \begin{nopar} + } + {% + \end{nopar} + \end{spacing} + \addvspace{\aa@afteracknowledgementsskip} + } +\let\acknowledgement\acknowledgements +\let\endacknowledgement\endacknowledgements +\renewcommand\@makefntext[1]{% + \noindent + \hb@xt@\bibindent{\hss\@makefnmark\enspace}#1} +\newcommand\listofobjects{\if@myobjects% + \section*{\listobjectname} + \@starttoc{obj}\fi% +} +\newcommand*\l@obj[2]{\noindent`#1' on page #2\par} +\DeclareRobustCommand{\object}[1]{% + #1\global\let\if@myobjects\iftrue% + \addcontentsline{obj}{obj}{#1}% +} +\newcommand\longtab[2][]{% +\if!\@aatolm! + \aalongfloat{table}{#2}% +\else + \aalongfloat[#1]{section}{#2}% +\fi +} +\newcommand\aalongfloat[3][]{% + \AtEndDocument{% + \aa@savecounter \csname c@#2\endcsname \relax + \csname c@#2\endcsname + }% + \edef\aa@nombre{\number\csname c@#2\endcsname}% +\if!\@aatolm! + \expandafter\AtEndDocument\expandafter{% + \aa@nombre\relax + \setlength{\LTcapwidth}{\textwidth} + \onecolumn + #3% + \twocolumn + \csname c@#2\endcsname \aa@savecounter \relax + }% + \stepcounter{#2}% +\else + \expandafter\AtEndDocument\expandafter{% + \aa@nombre\relax + \setlength{\LTcapwidth}{\textwidth} + \onecolumn +\setcounter{table}{#1}\addtocounter{table}{-1} +\renewcommand\thesection{\Alph{section}}% +\renewcommand\thetable{\thesection.\arabic{table}} + #3% + \twocolumn + \csname c@#2\endcsname \aa@savecounter \relax + }% + \setcounter{table}{#1} +\fi +} +\renewcommand*\enddocument{% + \let\AtEndDocument\@firstofone + \@enddocumenthook + \clearpage + \advance\c@page \m@ne + \immediate\write\@auxout{\string\newlabel{LastPage}{{\thepage}{\thepage}{}{}{}}} + \@checkend{document}% + \clearpage + \begingroup + \if@filesw + \immediate\closeout\@mainaux + \let\@setckpt\@gobbletwo + \let\@newl@bel\@testdef + \@tempswafalse + \makeatletter \input\jobname.aux + \fi + \@dofilelist + \ifdim \font@submax >\fontsubfuzz\relax + \@font@warning{Size substitutions with differences\MessageBreak + up to \font@submax\space have occurred.\@gobbletwo}% + \fi + \@defaultsubs + \@refundefined + \if@filesw + \ifx \@multiplelabels \relax + \if@tempswa + \@latex@warning@no@line{Label(s) may have changed. + Rerun to get cross-references right}% + \fi + \else + \@multiplelabels + \fi + \fi + \endgroup + \deadcycles\z@\@@end} +\newcommand*\aa@defineentry{% + \newcommand{\entry}[3]{% + \par\noindent + {\aa@entryiifont ##2}% + \par + {% + \noindent + \raggedright + {\aa@entryifont ##1}% + \hfill + \rlap{\makebox[\aa@entryboxwidth][l]{\hfill##3}}% + \par + }% + \vspace{\aftertext} + } +} +\ifaa@contents \aa@defineentry \fi +\ifaa@contentsAut \aa@defineentry \fi +\renewcommand\@listi{% + \leftmargin \leftmargini + \parsep \z@ \@plus\p@ \@minus\p@ + \topsep 8\p@ \@plus2\p@ \@minus4\p@ + \itemsep \parsep +} +\let\listI\@listi +\@listi +\AtBeginDocument{% + \let\@listi\listI + \@listi +} +\renewcommand\@listii{% + \leftmargin \leftmarginii + \labelwidth \leftmarginii + \advance\labelwidth -\labelsep + \topsep \z@ + \parsep \z@ + \itemsep \z@ +} +\renewcommand\@listiii{% + \leftmargin \leftmarginiii + \labelwidth \leftmarginiii + \advance\labelwidth -\labelsep + \topsep \z@ + \parsep \z@ + \itemsep \z@ + \partopsep \p@ \@minus\p@ + } +\newcommand*\aa@setitemindent[1]{% + \settowidth{\labelwidth}{\aa@descriptionlabelfont #1}% + \leftmargini \labelwidth + \advance\leftmargini \labelsep + \renewcommand*\@listi{% + \leftmargin \leftmargini + \labelwidth \leftmargini + \advance\labelwidth -\labelsep + \parsep \parskip + \topsep \medskipamount + \itemsep \parskip + \advance\itemsep -\parsep + }% +} +\newcommand*\aa@setitemitemindent[1]{% + \settowidth{\labelwidth}{\aa@descriptionlabelfont #1}% + \leftmarginii \labelwidth + \advance\leftmarginii \labelsep + \renewcommand*\@listii{% + \leftmargin \leftmarginii + \labelwidth \leftmarginii + \advance\labelwidth -\labelsep + \parsep \parskip + \topsep \z@ + \itemsep \parskip + \advance\itemsep -\parsep + }% +} +\renewcommand*\descriptionlabel[1]{\hspace\labelsep #1\hfil} +\renewcommand*\description{% + \@ifnextchar[{\aa@description} % ] (pour Emacs) + {% + \list{}{% + \labelwidth\z@ + \itemindent -\leftmargin + \let\makelabel\descriptionlabel + }% + }% +} +\newcommand\aa@description[1][]{% + \relax\ifnum\@listdepth=0 + \aa@setitemindent{#1}% + \else\ifnum\@listdepth=1 + \aa@setitemitemindent{#1}% + \fi\fi + \list{--}{\let\makelabel\aa@descriptionlabel}% +} +\newcommand*\aa@descriptionlabel[1]{% + \aa@descriptionlabelfont + #1% + \hfil +} +\newcommand*\aa@theorem@aftercount{.} +\newcommand*\aa@theorem@aftertitle{.} +\renewcommand*\newtheorem{% + \@ifstar{\aa@theorem@withstar}{\aa@theorem@nostar}% +} +\newcommand*\aa@theorem@nostar{% + \aa@numberedtheoremtrue + \aa@newtheorem +} +\newcommand*\aa@theorem@withstar{% + \aa@numberedtheoremfalse + \aa@newtheorem +} +\newcommand*\aa@newtheorem[1]{% + \def\aa@theorem@name{#1}% + \expandafter\newif\csname ifaa@theorem@#1@numbered\endcsname + \ifaa@numberedtheorem + \csname aa@theorem@#1@numberedtrue\endcsname + \fi + \aa@@newtheorem +} +\newif\ifaa@newcounter +\newcommand*\aa@@newtheorem[2][]{% + \def\aa@arg{#1}% + \ifx\aa@arg\empty + \expandafter\edef + \csname aa@theorem@\aa@theorem@name @counter\endcsname + {AA\aa@theorem@name}% + \aa@newcountertrue + \else + \expandafter\ifx + \csname aa@theorem@#1@title\endcsname + \relax + \ClassError{aa} + {#1 isn't a theorem-like environment} + {You have to create #1 with \string\newtheorem\space + before use its counter.}% + \expandafter\edef + \csname aa@theorem@\aa@theorem@name @counter\endcsname + {AA\aa@theorem@name}% + \aa@newcountertrue + \else + \expandafter\def + \csname aa@theorem@\aa@theorem@name @counter\endcsname + {AA#1}% + \aa@newcounterfalse + \fi + \fi + \expandafter\newcommand + \csname aa@theorem@\aa@theorem@name @title\endcsname + {#2}% + \aa@@@newtheorem +} +\newcommand*\aa@@@newtheorem[3][]{% + \ifaa@newcounter + \def\aa@arg{#1}% + \ifx\aa@arg\empty + \newcounter{\csname aa@theorem@\aa@theorem@name @counter\endcsname}% + \else + \newcounter{\csname aa@theorem@\aa@theorem@name @counter\endcsname}[#1]% + \expandafter\xdef + \csname theaa@theorem@\aa@theorem@name @counter\endcsname{% + \expandafter\noexpand\csname the#1\endcsname.% + \noexpand\arabic{aa@theorem@\aa@theorem@name @counter}% + }% + \fi + \fi + \expandafter\newcommand + \csname aa@theorem@\aa@theorem@name @titlefont\endcsname{#2}% + \expandafter\newcommand + \csname aa@theorem@\aa@theorem@name @bodyfont\endcsname{#3}% + \newenvironment{\aa@theorem@name}[1][]{% + \def\aa@theorem@optionnal{##1}% + \par\addvspace{\VSpaceBeforeTheorem}% + \noindent\hspace*{\HSpaceIndentTheorem}% + \begingroup + \csname aa@theorem@\@currenvir @titlefont\endcsname + \csname aa@theorem@\@currenvir @title\endcsname + \csname ifaa@theorem@\@currenvir @numbered\endcsname + \refstepcounter{\csname aa@theorem@\@currenvir @counter\endcsname}% + \space + \csname the\csname aa@theorem@\@currenvir @counter\endcsname\endcsname + \fi + \ifx\aa@theorem@optionnal\empty + \aa@theorem@aftercount + \else + \space(\aa@theorem@optionnal)% + \aa@theorem@aftertitle + \fi + \endgroup + \ifdim\HVSpaceSepTheorem<\z@ + \par\nobreak + \vspace{-\HVSpaceSepTheorem}% + \noindent\hspace*{\HSpaceIndentTheorem}% + \else + \hspace*{\HVSpaceSepTheorem}% + \fi + \csname aa@theorem@\@currenvir @bodyfont\endcsname + }% + {% + \par\addvspace{\VSpaceAfterTheorem} + }% +} +\newtheorem*{proof}{Proof}{\itshape}{\rmfamily} +\newtheorem{theorem}{Theorem}[section]{\bfseries}{\itshape} +\newtheorem{corollary}[theorem]{Corollary}{\bfseries}{\itshape} +\newtheorem{definition}[theorem]{Definition}{\bfseries}{\rmfamily} +\newtheorem{example}[theorem]{Example}{\itshape}{\rmfamily} +\newtheorem{exercise}[theorem]{Exercise}{\itshape}{\rmfamily} +\newtheorem{lemma}[theorem]{Lemma}{\bfseries}{\itshape} +\newtheorem{note}[theorem]{Note}{\itshape}{\rmfamily} +\newtheorem{problem}[theorem]{Problem}{\itshape}{\rmfamily} +\newtheorem{proposition}[theorem]{Proposition}{\bfseries}{\itshape} +\newtheorem{question}[theorem]{Question}{\itshape}{\rmfamily} +\newtheorem{remark}[theorem]{Remark}{\itshape}{\rmfamily} +\newtheorem{solution}[theorem]{Solution}{\itshape}{\rmfamily} +\setlength{\textfloatsep}{18\p@ \@plus 2\p@ \@minus 4\p@} +\setlength{\dbltextfloatsep}{18\p@ \@plus 2\p@ \@minus 4\p@} +\setlength{\@fptop}{\z@} +\setlength{\@fpsep}{12\p@} +\setlength{\@dblfptop}{\z@} +\setlength{\@dblfpsep}{12\p@} +\setcounter{topnumber}{4} +\renewcommand*\topfraction{.9} +\setcounter{bottomnumber}{2} +\renewcommand*\bottomfraction{.5} +\setcounter{totalnumber}{6} +\renewcommand*\textfraction{.05} +\renewcommand*\floatpagefraction{.95} +\setcounter{dbltopnumber}{3} +\renewcommand*\dbltopfraction{.9} +\renewcommand*\dblfloatpagefraction{.95} +\renewcommand*\fps@figure{tbp} +\renewcommand*\fps@table{tbp} +\def\sidecaption#1\caption{% + \setbox0=\hbox{\ignorespaces#1\unskip}% + \aa@sidecaptionwidth=\linewidth + \advance\aa@sidecaptionwidth -\wd0 + \advance\aa@sidecaptionwidth -\aa@figgap + \ifdim\aa@sidecaptionwidth<\aa@sidecaptionminwidth + \ClassWarning{aa}{% + No sufficient room for the legend; + using normal \string\caption.% + }% + \let\aa@caption\@caption + \unhbox0 + \else + \let\aa@caption\aa@sidecaption + \dimen0 \dp0 + \advance\dimen0 \ht0 + \dp0 \dp\strutbox + \advance\dimen0-\dp0 + \ht0 \dimen0 + \unhbox0\hspace{\aa@figgap}% + \fi + \refstepcounter\@captype + \@dblarg{\aa@caption\@captype}% +} +\long\def\aa@sidecaption#1[#2]#3{% + \addcontentsline + {\csname ext@#1\endcsname} + {#1} + {\protect\numberline{\csname the#1\endcsname}{\ignorespaces #2}}% + \begingroup + \@parboxrestore + \aa@makesidecaption{\csname fnum@#1\endcsname}{\ignorespaces #3}% + \par + \endgroup +} +\newcommand*\aa@capstrut{% + \leavevmode + \vrule \@width\z@ \@height\ht\strutbox \@depth\z@ +} +\def\aa@@makecaption#1{% + {\aa@headcaptionfont #1\aa@floatcounterend}% +} +\long\def\aa@makesidecaption#1#2{% + \parbox[b]{\aa@sidecaptionwidth}{% + \aa@captionfont + \aa@@makecaption{#1} + \aa@capstrut + #2% + }% +} +\renewcommand\@makecaption[2]{% + \aa@captionfont + \ifx\@captype\aa@figtype + \par\vskip\VSpaceBeforeFigCaption + \aa@@makecaption{#1}% + \aa@capstrut% + #2% + \par + \else + {\aa@headcaptionfont #1\aa@floatcounterend}% + \aa@capstrut + #2% + \par + \vskip\VSpaceAfterTabCaption + \fi +} +\newcommand\tablebib[1]{\VSpaceBeforeTabFoot=1ex% + \par\vspace{\VSpaceBeforeTabBib} + \noindent + \begin{minipage}{\linewidth} + {\aa@tablebibnamefont\aa@tablebibname.}~% + \aa@tablebibfont + \ignorespaces + #1% + \end{minipage}% +} +\newcommand\tablefoot[1]{\VSpaceBeforeTabBib=1ex% + \par\vspace{\VSpaceBeforeTabFoot} + \noindent + \begin{minipage}{\linewidth} + {\aa@tablefootnamefont\aa@tablefootname.}~% + \aa@tablefootfont + \ignorespaces + #1% + \end{minipage}% +} +\newcommand*\tablefootmark[1]{% + \unskip + \hbox{\@textsuperscript{\normalfont\itshape\ignorespaces#1}}% + \,% + \ignorespaces +} +\newcommand\tablefoottext[2]{% + \hbox{\@textsuperscript{\normalfont({\itshape\ignorespaces#1})}}% + ~% + \ignorespaces + #2\ \ignorespaces% +} +\setlength\bibindent{1em} +\renewenvironment{thebibliography}[1]{% + \begingroup + \section*{\refname}% + \@mkboth{\refname}{\refname}% + \aa@bibliographyfont + \list{\@biblabel{\@arabic\c@enumiv}}% + {% + \settowidth\labelwidth{\@biblabel{#1}}% + \ifaa@bibnumber + \leftmargin\labelwidth + \advance\leftmargin\labelsep + \else + \leftmargin\bibindent + \setlength{\itemindent}{-\leftmargin} + \fi + \@openbib@code + \usecounter{enumiv}% + \let\p@enumiv\@empty + \renewcommand\theenumiv{\@arabic\c@enumiv}% + }% + \sloppy + \clubpenalty4000 + \@clubpenalty \clubpenalty + \widowpenalty4000% + \sfcode`\.\@m +}{% + \endlist\par\endgroup% + \ifaa@longauth\kern6pt\hrule\kern6pt\aainstitutename\aa@longauthfalse\fi% + \ifaa@referee\if!\csname appendix\endcsname!\relax\else\listofobjects\fi\fi + \def\@noitemerr{\ClassWarning{aa}{Empty `thebibliography' environment}}% +} +\def \@floatboxreset {% + \reset@font + \ifx\@captype\aa@tabtype + \small + \spacetab + \fi + \@setnobreak + \@setminipage +} +\def\spacetab{% +\abovedisplayshortskip-10pt% +\belowdisplayshortskip0pt% +} +\DeclareRobustCommand{\ion}[2]{\textup{#1\,\textsc{\lowercase{#2}}}} +\newcommand*\element[1][]{% + \def\aa@element@tr{#1}% + \aa@element +} +\newcommand*\aa@element[1][]{% + \def\aa@element@tl{#1}% + \aa@@element +} +\newcommand*\aa@@element[1][]{% + \def\aa@element@bl{#1}% + \aa@@@element +} +\newcommand*\aa@@@element[2][]{% + \def\aa@element@br{#1}% + \ensuremath{% + \vphantom{x}^{\aa@element@tl}_{\aa@element@bl} + \mathrm{#2} + \vphantom{x}^{\aa@element@tr}_{\aa@element@br} + }% +} +\renewcommand*\vec[1]{\ensuremath{\boldsymbol{#1}}} +\newcommand*\tens[1]{\ensuremath{\mathsf{#1}}} +\newcommand*\sq{% + \ifmmode + \Box + \else + \begingroup + \unskip\nobreak + \hfil + \penalty50 + \hskip1em + \null\nobreak\hfil$\Box$% + \parfillskip=0pt + \finalhyphendemerits=0 + \endgraf + \endgroup + \fi +} +\newcommand*\sun{\ensuremath{\odot}} +\newcommand*\degr{\ensuremath{^\circ}} +\newcommand*\arcmin{\ensuremath{^\prime}} +\newcommand*\arcsec{\ensuremath{^{\prime\prime}}} +\def\utw{\ensuremath{\smash{\rlap{\lower5pt\hbox{$\sim$}}}}} +\def\udtw{\ensuremath{\smash{\rlap{\lower6pt\hbox{$\approx$}}}}} +\newcommand*\fd{\ensuremath{\overset{\text{d}}{.}}} +\newcommand*\fh{\ensuremath{\overset{\text{h}}{.}}} +\newcommand*\fm{\ensuremath{\overset{\text{m}}{.}}} +\newcommand*\fs{\ensuremath{\overset{\text{s}}{.}}} +\newcommand*\fdg{\ensuremath{\overset{\circ}{.}}} +\newcommand*\farcm{\ensuremath{\overset{\prime}{.}}} +\newcommand*\farcs{\ensuremath{\overset{\prime\prime}{.}}} +\newcommand*\fp{\ensuremath{\overset{\scriptscriptstyle\text{p}}{.}}} +\newcommand*\cor{\ensuremath{\mathrel{\widehat{=}}}} +\newcommand*\aa@centerstack[2]{% + \ensuremath{% + \mathrel{% + \mathchoice{% + \vcenter{% + \offinterlineskip + \halign{\hfil$\displaystyle##$\hfil\cr#1\cr#2\cr}% + }% + } + {% + \vcenter{% + \offinterlineskip + \halign{\hfil$\textstyle##$\hfil\cr#1\cr#2\cr}% + }% + } + {% + \vcenter{% + \offinterlineskip + \halign{\hfil$\scriptstyle##$\hfil\cr#1\cr#2\cr}% + }% + } + {% + \vcenter{% + \offinterlineskip + \halign{\hfil$\scriptscriptstyle##$\hfil\cr#1\cr#2\cr}% + }% + }% + }% + }% +} +\newcommand*\la{\aa@centerstack{<}{\sim}} +\newcommand*\ga{\aa@centerstack{>}{\sim}} +\newcommand*\sol{\aa@centerstack{\sim}{<}} +\newcommand*\sog{\aa@centerstack{\sim}{>}} +\newcommand*\lse{\aa@centerstack{<}{\simeq}} +\newcommand*\gse{\aa@centerstack{>}{\simeq}} +\newcommand*\aa@centerstackskip[6]{% + \ensuremath{% + \mathrel{% + \mathchoice{% + \vcenter{% + \offinterlineskip + \halign{\hfil$\displaystyle##$\hfil\cr + #1\cr\noalign{\vskip#3}#2\cr}% + }% + } + {% + \vcenter{% + \offinterlineskip + \halign{\hfil$\textstyle##$\hfil\cr + #1\cr\noalign{\vskip#4}#2\cr}% + }% + } + {% + \vcenter{% + \offinterlineskip + \halign{\hfil$\scriptstyle##$\hfil\cr + #1\cr\noalign{\vskip#5}#2\cr}% + }% + } + {% + \vcenter{% + \offinterlineskip + \halign{\hfil$\scriptscriptstyle##$\hfil\cr + #1\cr\noalign{\vskip#6}#2\cr}% + }% + }% + }% + }% +} +\newcommand*\grole{\aa@centerstackskip{>}{<}{-1.5\p@}{-1.5\p@}{-1\p@}{-.5\p@}} +\newcommand*\leogr{\aa@centerstackskip{<}{>}{-1.5\p@}{-1.5\p@}{-1\p@}{-.5\p@}} +\newcommand*\loa{\aa@centerstack{<}{\approx}} +\newcommand*\goa{\aa@centerstack{>}{\approx}} +\newcommand*\diameter{% + \ensuremath{% + \mathchoice{% + \ooalign{% + \hfil\hbox{$\displaystyle/$}\hfil\crcr + {\hbox{$\displaystyle\mathchar"20D$}}% + }% + } + {% + \ooalign{% + \hfil\hbox{$\textstyle/$}\hfil\crcr + {\hbox{$\textstyle\mathchar"20D$}}% + }% + } + {% + \ooalign{% + \hfil\hbox{$\scriptstyle/$}\hfil\crcr + {\hbox{$\scriptstyle\mathchar"20D$}}% + }% + } + {% + \ooalign{% + \hfil\hbox{$\scriptscriptstyle/$}\hfil\crcr + {\hbox{$\scriptscriptstyle\mathchar"20D$}}% + }% + }% + }% +} +\let\olddiameter\diameter +\newcommand*\getsto{\aa@centerstack{\gets}{\to}} +\newcommand*\lid{\aa@centerstackskip{<}{=}{1.2\p@}{1.2\p@}{1\p@}{0.9\p@}} +\newcommand*\gid{\aa@centerstackskip{>}{=}{1.2\p@}{1.2\p@}{1\p@}{0.9\p@}} +\newcommand*\bbbone{% + \ensuremath{% + \mathchoice{\mathrm 1\mskip-4mu l} + {\mathrm 1\mskip-4mu l} + {\mathrm 1\mskip-4.5mu l} + {\mathrm 1\mskip-5mu l}% + }% +} +\newcommand*\aap{A\&A} +\let\astap=\aap +\newcommand*\aapr{A\&A~Rev.} +\newcommand*\aaps{A\&AS} +\newcommand*\actaa{Acta Astron.} +\newcommand*\aj{AJ} +\newcommand*\ao{Appl.~Opt.} +\let\applopt\ao +\newcommand*\apj{ApJ} +\newcommand*\apjl{ApJ} +\let\apjlett\apjl +\newcommand*\apjs{ApJS} +\let\apjsupp\apjs +\newcommand*\aplett{Astrophys.~Lett.} +\newcommand*\apspr{Astrophys.~Space~Phys.~Res.} +\newcommand*\apss{Ap\&SS} +\newcommand*\araa{ARA\&A} +\newcommand*\azh{AZh} +\newcommand*\baas{BAAS} +\newcommand*\bac{Bull. astr. Inst. Czechosl.} +\newcommand*\bain{Bull.~Astron.~Inst.~Netherlands} +\newcommand*\caa{Chinese Astron. Astrophys.} +\newcommand*\cjaa{Chinese J. Astron. Astrophys.} +\newcommand*\fcp{Fund.~Cosmic~Phys.} +\newcommand*\gca{Geochim.~Cosmochim.~Acta} +\newcommand*\grl{Geophys.~Res.~Lett.} +\newcommand*\iaucirc{IAU~Circ.} +\newcommand*\icarus{Icarus} +\newcommand*\jcap{J. Cosmology Astropart. Phys.} +\newcommand*\jcp{J.~Chem.~Phys.} +\newcommand*\jgr{J.~Geophys.~Res.} +\newcommand*\jqsrt{J.~Quant.~Spectr.~Rad.~Transf.} +\newcommand*\jrasc{JRASC} +\newcommand*\memras{MmRAS} +\newcommand*\memsai{Mem.~Soc.~Astron.~Italiana} +\newcommand*\mnras{MNRAS} +\newcommand*\na{New A} +\newcommand*\nar{New A Rev.} +\newcommand*\nat{Nature} +\newcommand*\nphysa{Nucl.~Phys.~A} +\newcommand*\pasa{PASA} +\newcommand*\pasj{PASJ} +\newcommand*\pasp{PASP} +\newcommand*\physrep{Phys.~Rep.} +\newcommand*\physscr{Phys.~Scr} +\newcommand*\planss{Planet.~Space~Sci.} +\newcommand*\pra{Phys.~Rev.~A} +\newcommand*\prb{Phys.~Rev.~B} +\newcommand*\prc{Phys.~Rev.~C} +\newcommand*\prd{Phys.~Rev.~D} +\newcommand*\pre{Phys.~Rev.~E} +\newcommand*\prl{Phys.~Rev.~Lett.} +\newcommand*\procspie{Proc.~SPIE} +\newcommand*\qjras{QJRAS} +\newcommand*\rmxaa{Rev. Mexicana Astron. 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+\documentclass{aa} +\usepackage{lscape} +\usepackage{longtable,threeparttable} +\usepackage{graphicx} +\usepackage{txfonts} +\usepackage{caption} +\usepackage{subcaption} +\usepackage{hyperref} +\usepackage[normalem]{ulem} +\usepackage{soul} +\usepackage{color} +\hypersetup{ + unicode=true, + pdftoolbar=true, + pdfmenubar=true, + pdffitwindow=false, + pdfstartview={FitH}, + pdftitle={My title}, + pdfauthor={Author}, + pdfsubject={Subject}, + pdfcreator={Creator}, + pdfproducer={Producer}, + pdfkeywords={keyword1, key2, key3}, + pdfnewwindow=true, + colorlinks=true, + linkcolor=blue, + citecolor=blue, + filecolor=magenta, + urlcolor=blue +} +\newcommand {\Fig}{Fig\,} + +\begin{document} + + + \title{From synthetic SEDs to stellar origins: A deep learning model for physical parameter retrieval in hot subdwarf stars} + \titlerunning{Deep learning SED modeling of hot subdwarfs} + + \author{Mengqi Feng\inst{1} + \and + Zhenxin Lei\inst{1}\fnmsep\thanks{e-mail: \href{mailtoleizhenxin2060@163.com} + {leizhenxin2060@163.com}} + \and + Bokai Kou \inst{1} + \and + Yangyang Dong\inst{1} + \and + Ke Hu\inst{1} + \and + Huaping Xiao\inst{1} + \and + Jingkun Zhao\inst{2} + } + + \institute{Key Laboratory of Stars and Interstellar Medium, Xiangtan University, Xiangtan 411105, People's Republic of China. + \and + Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China. + } + + \authorrunning{Feng et al.} + \abstract + % context heading (optional) + {} + % aims heading (mandatory) +{The formation mechanisms of spectrally diverse hot subdwarfs remain unclear. While existing mass distribution analyses suggest additional channels beyond helium white dwarf (He-WD) mergers contribute to He-rich subdwarf formation, these conclusions are constrained by the limited sample sizes of mass-measured He-rich objects.} + % methods heading (mandatory) +{We developed a deep leaning model that combines a convolution neural network (CNN) with a squeeze-and-excitation (SE) block to calculate synthetic spectral energy distributions (SEDs) for 1,012 spectroscopically confirmed hot subdwarfs.\LEt{***A&A style leans towards the use of that when providing essential and defining information about a subject because it is a more direct expression of the relationship between the subject and the description. If you'd like to see examples, I'd suggest referring to Sect. 8.3 of our English Guide.} By directly comparing synthetic SEDs and the observed flux density, we derived stellar parameters (mass, radius, and luminosity) for an unprecedented number of hot subdwarf stars, enabling more conclusive channel discrimination than prior studies.} + % results heading (mandatory) +{The mass distribution of sdB/sdOB stars confirmed the results from model predictions of binary population synthesis (BPS). A primary and secondary peak (i.e., around 0.56 and 0.4 ${\rm M}_{\odot}$) is obviously presented in the mass distribution of He-rich hot subdwarf stars. By comparing this with the results from the predictions of the recent BPS model, we propose that the merger of two He-WDs could produce most of the observed He-rich hot subdwarf stars, but the mass transfer during the stable Roche lobe overflow phase in binary evolution should be partially conserved.} + % conclusions heading (optional), leave it empty if necessary + {} + {} + + \keywords{(Stars:) subdwarfs; + binaries (including multiple): close; + Stars: evolution; + Stars: fundamental parameters + } + + \maketitle +% +%________________________________________________________________ + +\section{Introduction} +Hot subdwarf stars are positioned between main-sequence (MS) and white dwarf (WD) regions in the Hertzsprung-Russell diagram (HRD) \citep{1986A&Aheber}. Hot subdwarf stars have very low stellar masses (e.g., 0.5 ${\rm M}_{\odot}$) and thin envelopes ($M_{\text{env}} \le 0.02 M_{\odot}$), but exhibit very high effective temperatures (e.g., $20,000~\mathrm{K} \leq T_{\text{eff}} \leq 70,000~\mathrm{K}$) and large surface gravities (e.g., $5.0 \leq \log g \leq 6.5$). These blue stars have a diversity of atmospheric compositions that could present atmospheres from pure hydrogen (H) to pure helium (He). According to their spectral line features, hot subdwarfs can be classified into sdB, sdO, sdOB, He-sdB, He-sdO, and He-sdOB types \citep{1990_A&AS_moehler,2017_A&A_geier, 2018ApJ...868...70L}. In addition, \citet{2013A&A...551A..31D} designed an MK-like classification scheme by which hot subdwarf stars could be classified in a similar way as normal MS stars (also see \citealt{2021MNRAS.501..623J, 2024PASJ...76.1084Z}). SdB stars are also referred to as extreme horizontal branch (EHB) stars due to their location at the bluest end of the horizontal branch (HB +). More characteristics of hot subdwarf stars were described in recent excellent reviews of \citet{2009ARA&A..47..211H, 2016PASPHeber}. + +Generally, single stars with such low stellar masses as hot subdwarfs cannot evolve into core He burning or even a late stage within Hubble time. Although formation channels connected with single stars were proposed by several authors (\citealt{1993ApJ...407..649C, 2008A&A...491..253M}), \citet{2020A&A...642A.180P} found that binary interactions are always required in the formation of hot subdwarf stars, including those in wide binary systems. +Furthermore, most of the sdB-type hot subdwarfs were found in close binaries \citep{2001MNRASmaxted, 2004Ap&SSnapiwotzki,2011MNRAScopperwheat, 2025A&A...693A.121H}. These results indicate that binary evolution could provide natural explanations for the formation of hot subdwarfs. + +\citet{2002MNRASHan, 2003MNRASHan} investigated the characteristics of hot subdwarfs formed through binary evolution using the binary population synthesis (BPS) method. They found that stable Roche lobe overflow (RLOF), common envelope (CE) ejection, and the merger of two helium white dwarfs (He-WDs) could produce sdB stars in long-period binaries, short-period binaries, and single sdB stars, respectively.\LEt{***A&A uses the serial (Oxford) comma between three or more items in a list to avoid confusion. Also use commas after introductory sentences of three or more words. Commas are not necessary between just two parallel items in a sentence.} Most of the observed characteristics for sdB stars could be satisfied by their model predictions. \citet{2012MNRASZhang} and \citet{2017ApJ...835..242Z} studied in detail the mergers of two He-WDs and a WD + MS star, respectively. They found that both channels could produce He-rich sdB stars such that their observed features could be satisfied. +In addition, \citet{2022MNRASmiller} proposed that the merger of carbon-oxygen WDs with He WDs could form He-rich hot subdwarfs with atmospheres strongly enriched by carbon and oxygen. Recently, \citet{2021MNRAS.507.4603M} and \citet{2024RAA....24e5003J} proposed that the MS companion of massive WD could survive the type Ia supernova (SN) explosions and become intermediate He-rich hot subdwarf stars if their envelopes are ejected during the explosion. Their model predicted that the peak of mass distribution for survived stars is around 0.4 $\rm M_{\odot}$, which is consistent with the results in \citet{2023ApJLei}. However, the birth rate of this channel would be too low compared to the number of He-rich hot subdwarf stars discovered up to now \citep{2021MNRAS.507.4603M}. \citet{2024ApJ...964...22L} proposed that massive sdO/B stars could be produced from CE ejection process with an asymptotic giant branch (AGB) star. This model could explain the recently discovered sdO binary star SMSS-J1920 \citep{2022MNRAS.515.3370L}, for which strong Ca H and K lines are presented in its spectrum. + +With a large number of new hot subdwarf stars having been discovered using the new data release of spectroscopic surveys \citep{2017OAst...26..164G, 2019MNRAS.486.2169K, 2018ApJ...868...70L, 2019ApJ...881..135L, 2020ApJ...889..117L, 2023ApJ...942..109L, 2019ApJ...881....7L, 2021ApJS..256...28L,2019A&A...630A..80S, 2021MNRAS.501..623J}, also with the help of the Gaia mission Early Data Release 3 (Gaia EDR3, \citealt{2021A&A...649A...1G}), \citet{2022A&ACulpan} compiled two catalogs for known hot subdwarf stars and their candidates, respectively (also see the serial studies, \citealt{2017_A&A_geier, 2019A&A...621A..38G, 2020A&A...635A.193G}). The catalog of known hot subdwarfs contains more than 6000 identified hot subdwarf stars, in which more than 3000 stars have atmospheric parameters and 2,700 stars have radial velocities. The candidate catalog contains more than 60,000 objects, which can be used as reliable input catalogs for follow-up analysis with new observed data from spectroscopy. + +Driven by the availability of large observational datasets, machine learning has been extensively applied in astronomical research, including studies of hot subdwarfs. \citet{2019ApJbu} combined a convolution neural network (CNN) with a support vector machine (SVM) to classify hot subdwarf stars in the dataset of Large Sky Area Multi-Fiber Spectroscopic Telescope (LAMOST, \citealt{2012RAA....12.1197C, 2012RAA....12..723Z}). \citet{2022ApJStan} also used CNN to search for hot subdwarf candidates in a larger LAMOST spectra dataset. More recently, \citet{2024PASJliu} applied the machine learning method to identify hot subdwarfs using photometric data, while \citet{2024ApJSchen} constructed a Se-ResNet+SVM model to search for hot subdwarf stars and predicted their atmospheric parameters. + +Despite considerable progress having been made both in simulation and observation of hot subdwarf stars, questions remain regarding the formation channels for those stars. Some notable challenges stem from the determination of physical parameters, such as masses, radii, and luminosities. Accurate mass estimation methods include asteroseismology and Eclipse binary. However, their applications are limited by the strict requirements of observed data that only dozens of hot subdwarfs have accurate masses determined by these methods \citep{2012A&AFontaine}. To analyze the mass distribution of hot subdwarfs with different companion types, \citet{2022A&ASchaffenroth} obtained masses, radii, and luminosities for 68 hot subdwarf stars by comparing observed fluxes with synthetic fluxes calculated from spectral energy distributions (SEDs).\LEt{***Acronyms should be spelled out upon first appearance. All subsequent appearances should be in the acronym form (unless at the beginning of a sentence). Any acronyms that are defined in the abstract need to be re-introduced in the main text.} With the help of these parameters, and with the help of space-based light curves from the Transiting Exoplanet Survey Satellite (TESS, \citealt{2015JATIS...1a4003R}) and the K2 space mission \citep{2014PASP..126..398H}, \citet{2023A&A...673A..90S} further obtained the masses of 27 companions for these hot subdwarf binaries. + +Using a similar method, \citet{2023ApJLei} obtained masses, radii, and luminosities for 664 single-lined hot subdwarfs with the spectra of LAMOST. Based on this large size of sample, they obtained the mass distributions for hot subdwarf stars with different spectral types, and compared them with the results from model predictions. Although the mass distribution of sdB/sdOB stars is consistent with the prevailing model of \citet{2002MNRASHan, 2003MNRASHan}, they found that He-rich hot subdwarf stars have an obviously lower peak of mass distribution (e.g., around 0.42 ${\rm M}_{\odot}$) than model predictions (e.g., 0.5 - 0.6 ${\rm M}_{\odot}$, see \Fig 12 in \citealt{2023ApJLei}). Based on these comparisons, they proposed that besides the two He-WDs merging channel, there should be other important formation channels for He-rich hot subdwarfs. However, only 39 He-rich stars were used in their statistical analysis, and such a small size sample would influence the final conclusions. + +As a further study of \citet{2023ApJLei}, we constructed a deep learning architecture that integrates a CNN with a squeeze-and-excitation (SE) block to calculate the synthetic SEDs for more than 2000 known hot subdwarfs selected in \citet{2022A&ACulpan} with the spectra of LAMOST and Sloan Digital Sky Survey (SDSS, \citealt{2020ApJS..249....3A}). +Using these SEDs, we calculated the synthetic fluxes at stellar surface and compared them with fluxes observed on the Earth to obtain masses, radii, and luminosities for the selected hot subdwarf stars. These parameters were used in following statistical analysis to help us understand the formation of hot subdwarfs more deeply. The structure of this paper is as follows. Sample selection and methods are described in Section 2. Section 3 presents our main results. A detailed discussion for mass distribution with a large size of sample is given in Section 4. A brief summary in Section 5 closes this paper. + +\section{Methodology and sample selection} +\subsection{Deep learning model SENN } + +\begin{figure*} + \centering + \includegraphics[width=0.8\linewidth]{picture/SENN.pdf} + \caption{Structure of deep learning model SENN. See section 2.1 for detailed description.\LEt{***The first sentence of each figure caption or legend should be a descriptive title of the figure as a whole, written in a telegraphic style with the initial article (the, a, an) omitted. The text that follows should be written in complete sentences. If individual panels are described, this is repeated (another telegraphic description followed by full sentences).} } + \label{Fig 1} +\end{figure*} + +We designed a deep learning model, which integrates a CNN neural network with a SE block (hereafter SENN), to calculate synthetic SEDs for selected hot subdwarf stars.\LEt{***Single-sentence paragraphs should be avoided.} As is shown in \Fig \ref{Fig 1}, SENN accepts normalized stellar spectra with a shape of 2,984 $\times$ 1 as inputs, and processes them through a hierarchical architecture to calculate SEDs. The model comprises three modules. The initial feature embedding module uses a 1D convolution layer (64 filters, 3 kernels, and ReLU activation) to capture local spectral features, and reshape the output into a 64 $\times$ 2982 tensor. The SE feature refinement module is then employed, in which a global average pooling (GAP) layer compresses global spatial information into a channel-wise descriptor. This descriptor is connected by two dense layers to fully capture channel-wise dependencies and compute channel-specific weights. These weights are then applied to the original feature map, producing the final weighted feature map. Finally, the SED regression module is used to flatten the refined features, pass them through a 64-neuron dense layer, and generate SEDs through an output layer. + + The SENN model takes observed spectra as input features and their corresponding synthetic SEDs as training labels. Through training processes, SENN +established a mapping relationship between observed spectra and synthetic SEDs, enabling it to calculated the synthetic SED associated with a given observed spectrum. With these synthetic SED and the observed magnitudes retrieved from the virtual observatory (VO), we could calculate the masses, radii and luminosities of hot subdwarf stars reported in \citet{2022A&ACulpan}, if their atmospheric parameters are known (e.g., $T_{\text{eff}}$ and $\log g$. see Section 2.3).\LEt{***If this is the Spanish Virtual Observatory introduced later, please introduce the acronym here and only use the acronym henceforth.} + +\subsection{Training dataset} + +In previous studies (\citealt{2018ApJ...868...70L,2019ApJ...881..135L, 2020ApJ...889..117L, 2023ApJ...942..109L}), 950 single-lined hot subdwarf stars were identified with LAMOST spectra. Their atmospheric parameters, i.e., effective temperature ($T_{\text{eff}}$), surface gravity (${\rm log} g$), and logarithmic number ratio of helium to hydrogen ($\log(n_{\text{He}}/n_{\text{H}})$), were determined by fitting H and He profiles with synthetic spectra. The synthetic spectra and SEDs of these stars were generated using \texttt{Synspec} (version~49; \citealt{2007ApJSLanz}) with nonlocal thermodynamic equilibrium (NLTE) Tlusty atmospheres (version 204; \citealt{2017arXivHubeny}). See \citet{2018ApJ...868...70L} and \citet{2014ASPC..481...95N} for more details about the synthetic spectra and SED calculation. + +In this study, the synthetic SEDs of the 950 stars mentioned above were used as a training sample for the SENN model, while the observed spectra of these stars were adopted as SENN inputs.\LEt{***Verify that your intended meaning has not been changed.} 80\% of the selected stars were used as training dataset, while 20\% of them were used as test dataset.\LEt{***Avoid beginning a sentence with an acronym (especially a paragraph), and do not begin with a numeral, formula, or symbol.} + +\subsection{Known hot subdwarfs and their spectra} +\citet{2022A&ACulpan} compiled a catalog of the known hot subdwarf stars that contains 6,616 unique sources collected from the literature. This catalog provides atmospheric parameters for 3,087 stars and radial velocities for 2,791 stars. To obtain the observed spectra for these stars, we cross-matched the catalog with the dataset of LAMOST DR11 and SDSS DR18, and then totally obtained 4,289 spectra. After removing duplicated sources +and low-quality spectra (e.g., that had a signal-to-noise ratio in the u band of less than 5.0), 3,411 unique spectra of known hot subdwarfs were left. Since $T_{\text{eff}}$ and $\log g$ are necessary parameters to determine stellar masses and luminosities in this study, only stars with the two parameters reported in the catalog of \cite{2022A&ACulpan} were finally selected for the following analysis, and it contains 2047 hot subdwarf stars. + + Within the catalog of \citet{2022A&ACulpan}, the atmospheric parameters of hot subdwarfs were collected from different studies; these were predominantly derived through spectral fitting.\LEt{***Verify that your intended meaning has not been changed.} However, as we lack the specific atmospheric models and parameters used in these works to calculate synthetic spectra for hot subdwarf stars, we did not employ the conventional method of deriving the SEDs for this selected sample with known atmospheric parameters. Instead, we utilized the highly efficient SENN model to compute the SEDs for these hot subdwarfs with corresponding observed spectra. + +Using the SENN model constructed in Section 2.1 and the training dataset selected in Section 2.2, synthetic SEDs for 2047 selected hot subdwarf stars were calculated; these were then used to obtain stellar masses, radii, and luminosities, as is described in the next section. Note that the SENN model is much more efficient at calculating synthetic SEDs than traditional methods. For example, it just needs tens of seconds to obtain synthetic SEDs for 2000 stars, and would be more powerful when confronting with huge numbers of stars. + + In Fig \ref{Fig 2}, we compare the ‌synthetic SED of a hot subdwarf star calculated using the ‌SENN model (dashed blue curve) with that computed directly from the ‌Tlusty model (solid red curve). The near-identical agreement between the two SEDs ‌fully demonstrates that utilizing the deep learning method to calculate theoretical SEDs for hot subdwarfs is both ‌feasible and reliable. + + +\subsection{Determination of masses, radii, and luminosities for selected hot subdwarf stars} +Using the synthetic SEDs calculated by SENN model, we obtained the flux density at the stellar surface within a specific pass-band.\LEt{***Or possibly "within specific pass-bands."} The synthetic flux density can be compared with the flux density observed on the Earth to determine the stellar angular diameters. The synthetic flux density at stellar surface, observed flux density on the Earth, stellar angular diameter, radius, and distance of the star have the following relationships \citep{2018OAst...27...35H, 2023ApJLei}: +\begin{equation} + \frac{f\left ( \lambda \right ) }{F\left ( \lambda \right ) } =\frac{\theta ^{2} }{4} =\frac{R^{2} }{d^{2}} + \label{eq 1} +,\end{equation} + +where $f(\lambda)$ is the flux density observed on the Earth, +$F(\lambda)$ is the synthetic flux density at stellar surface, $\theta$ is the angular diameter of the star, $R$ is the radius of the star, and $d$ is the stellar distance from the Earth. + +If the distance of a star is known, the stellar radius can be determined according to Equation (1). Then, with the help of atmospheric parameters (e.g., $\log g$ and $T_{\text{eff}}$), we can obtain the mass and luminosity of the star using the following equations: + +\begin{align} +M & = \frac{gR^{2}}{G} \label{eq 2} \\ +\frac{L}{L_{\odot} } & = \left ( \frac{R}{R_{\odot}} \right ) ^{2}\left ( \frac{T_{\rm eff}}{T_{\odot}} \right ) ^{4} \label{eq 3} +,\end{align} + where $L_{\odot}$, $R_{\odot}$, and $T_{\odot}$ are the luminosity, radius, and effective temperature of the Sun, respectively. + +Distances for the stars selected in this study were calculated using Gaia DR3 parallaxes \citep{2023A&Agaiadr3} after zero-point correction \citep{2021A&A...649A...4L}. The flux density observed on the Earth were obtained by searching for photometric data using VO SED Analyzer (VOSA, \citealt{2008_A&A_bayo}) of the Spanish Virtual Observatory (SVO) and converting observed magnitudes into fluxes. + +When converting the observed magnitude into the corresponding observed flux on the Earth, an extinction correction must be applied. To determine the visual extinction, $A_{\rm V}$, we fit the synthetic SEDs with the observed fluxes by treating $A_{\rm V}$ as a free parameter. For each trial value of $A_{\rm V}$, the wavelength-dependent extinction, $A_\lambda$, was computed as +\begin{equation} +A_\lambda = A_{\rm V} \times (k_\lambda / k_V), +\end{equation} +where $k_\lambda / k_{\rm V}$ represents the normalized extinction law. The functional form of $k_\lambda / k_V$ was adopted from \citet{1999PASP..111...63F} with $R_{\rm V} = 3.1$ and $k_{\rm V} = 211.4$. The observed fluxes, $f_{\text{obs}}(\lambda)$, were then dereddened using +\begin{equation} +f(\lambda) = f_{\text{obs}}(\lambda) \times 10^{\,A_\lambda / 2.5}, +\end{equation} +which yielding the intrinsic flux density, $f(\lambda)$. The best-fit $A_{\rm V}$ were determined simultaneously through $\chi^2$ minimization between the dereddened fluxes and the synthetic SEDs. + +\begin{figure} + \centering + \includegraphics[width=1.0\linewidth]{picture/spec-57919-HD173133N504043V01_sp07-209.fits.pdf} + \caption{Comparison between the synthetic SED calculated with Tlusty model (solid red curve) and the SED calculated by SENN model (dashed blue curve). The bottom panel displays the residual differences between the two SEDs.} + \label{Fig 2} +\end{figure} + + Using the method described above, we obtained masses, radii, and luminosities for the selected 2,047 hot subdwarf stars. The stars with mass values lower than 0.1 $M_\odot$ or higher than 1.0 $M_\odot$ are not reported here, since these values could be significantly influenced by large uncertainties of input parameters, and are not reasonable for normal hot subdwarf stars. Furthermore, only stars with reliable parallaxes (e.g., $\sigma_{\varpi}/\varpi\leq$ 0.2) are included in the following analysis. Thus, we finally have 1,012 hot subdwarf stars for which the main parameters are reported in this study (see Table \ref{tab1}), consisting of 606 sdB, 64 sdO, 206 sdOB, 9 He-sdB, 66 He-sdO, and 61 He-sdOB stars, respectively.\LEt{***Verify that your intended meaning has not been changed.} The obtained parameter values are presented in Table \ref{tab1}. + + Using Monte Carlo methods, we obtained the statistical errors ($\sigma_{sta}$) for mass, radius, and luminosity of the selected stars. Specifically, we calculated the median values for the three parameters, along with their values at the 16th and 84th percentiles. This defines a 68\% confidence interval around the median values and provides the corresponding asymmetric uncertainties. + + On the other hand, we cross-matched the sample from this work with the sample from \citet{2022A&ASchaffenroth}, and identified 24 common sources. By comparing the masses, radii, and luminosities for these 24 sources, we determined the systematic errors ($\sigma_{sys}$), which were calculated using the following formula: +\begin{equation*} +\sigma_{sys}=\frac{\sum(x_{i}-y_{i}) }{N} +,\end{equation*} + where $x_{i}$ is the parameter value calculated in this work, $y_{i}$ is the parameter value calculated in \citet{2022A&ASchaffenroth}, and $N$ is the number of common sources. The final errors ($\sigma$) was then calculated as + \begin{equation} + \sigma=\sqrt{\sigma_{sta}^2+\sigma_{sys}^2} + .\end{equation}\LEt{***Equations in the main text should be followed by a comma or a period (full stop) when necessary, as if they were phrases forming part of a sentence.} + Using the method described above, we obtained systematic errors of ‌0.02 $\rm M_{\odot}$ , ‌0.002 $\rm R_{\odot}$, and ‌1.4 $\rm L_{\odot}$ for mass, radius and luminosity, respectively. In Table \ref{tab1}, we presented the ‌final errors for these three parameters, incorporating both statistical errors and systematic errors. + +\section{Results} +\subsection{Main parameters for selected hot subdwarf stars} + +\begin{figure*} + \centering + \includegraphics[width=0.85\linewidth]{picture/mass_vs_parameters.pdf} + \caption{Relationship between mass and atmospheric parameters for the selected hot subdwarfs. Labels with different colors indicate the spectral classification from \citet{2022A&ACulpan}.} + \label{Fig 3} +\end{figure*} + +The masses, radii, luminosities, and other important parameters for the 1,012 selected hot subdwarf stars are presented in Table \ref{tab1}. From left to right, it gives object names, Gaia source\_id, spectral classification, $T_{\text{eff}}$, ${\rm log} g$, extinction coefficient ($A_{\rm V}$), Gaia parallax after zero-point correction, and four parameters obtained in this study, i.e., angular diameter, radius, luminosity, and mass. Of these stars, 601 have had their masses reported in previous studies. This means that the masses of 411 hot subdwarfs are reported for the first time in this study. + +The four panels in \Fig \ref{Fig 3} present the relationships between obtained masses and atmospheric parameters; for example, from top left to bottom right, it gives planes of mass versus $T_{\text{eff}}$, ${\rm log} g$, $\log (n_{\text{He}}/n_{\text{H}})$, and $\log L$, respectively. It can be observed that most of the selected hot subdwarfs have radii of between 0.1 and 0.3 $\rm R_{\odot}$, luminosities between 0.5 and 2.5 $\rm L_{\odot}$, and masses between 0.2 and 0.8 ${\rm M}_{\odot}$, respectively. These results are consistent with those of \citet{2023ApJLei}; see also \Fig 3 in their study. + +\subsection{Comparison with previous study} +In order to evaluate the reliability of the masses, radii, and luminosities obtained in this study, we cross-matched the selected hot subdwarfs with the stars analyzed in \citet{2022A&ASchaffenroth} and \citet{2023ApJLei}, respectively. Comparisons of masses, radii, and luminosities for the common stars are shown in the panels of \Fig \ref{Fig 4}. As can be see in the figure, there is a notable agreement between the results of the present study and previous research, particularly with respect to radius and luminosity. However, the comparison of mass exhibits a slightly larger dispersion than the other two parameters.\LEt{***Verify that your intended meaning has not been changed.} This is mainly due to the fact that the large uncertainties of surface gravity would directly influence stellar mass determination (see Equation \ref{eq 2}), while it is not used in the determination of radius and luminosity (see Equation \ref{eq 1} and \ref{eq 3}). +\begin{figure*} + \centering + \includegraphics[width=0.3\linewidth]{picture/contrast_Schaffenroth_radius.pdf} + \includegraphics[width=0.3\linewidth]{picture/contrast_Schaffenroth_mass.pdf} + \includegraphics[width=0.3\linewidth]{picture/contrast_Schaffenroth_lumin.pdf} + + \includegraphics[width=0.3\linewidth]{picture/contrast_Lei_radius.pdf} + \includegraphics[width=0.3\linewidth]{picture/contrast_Lei_mass.pdf} + \includegraphics[width=0.3\linewidth]{picture/contrast_Lei_lumin.pdf} + \caption{Top panels: Comparison of radii, masses, and luminosities between this study and \citet{2022A&ASchaffenroth}. Bottom panels: Comparison of radii, masses, and luminosities between this study and \citet{2023ApJLei}. } + \label{Fig 4} +\end{figure*} + +\subsection{Mass distribution of hot subdwarf stars} + +\begin{figure*} + \centering + \includegraphics[width=0.45\linewidth]{picture/distribute_mass_plx.pdf} + \includegraphics[width=0.45\linewidth]{picture/distribute_mass_logg.pdf} + \caption{Mass distribution for selected hot subdwarfs with different precisions of parallax (left panel) and surface gravity (right panel). See context for details.}\LEt{***"context" or "contexts" does not sound right here. Perhaps you mean "See main text" or "See commentary"} + \label{Fig 5} +\end{figure*} + +Since the precision of masses obtained in this study depends mainly on the precision of the parallax (i.e., distance) and surface gravity, we show the mass distribution with different uncertainties of parallax and surface gravity in \Fig \ref{Fig 5}. In the left panel, the entire sample has been split into three groups according to the relative parallax uncertainty (e.g., $\sigma_{\varpi}/\varpi\leq$ 0.2, 0.1 and 0.05, respectively). As expected, with the parallax precision increasing from 0.2 to 0.05, the number of hot subdwarf stars in each mass bin decreases. However, the three groups of hot subdwarfs show very similar mass distributions. As can be seen, all groups have a wide mass range of 0.1 - 1.0 ${\rm M}_{\odot}$ and present two distinct peaks: a primary peak at 0.47 ${\rm M}_{\odot}$ and a secondary peak at 0.37 ${\rm M}_{\odot}$ (see detailed discussion on the mass distribution in Section 4). On the other hand, the entire sample has been separated into three other groups in the right panel according to the relative uncertainty of surface gravity (e.g., uncertainty of ${\rm log} g$ over ${\rm log} g$ less than 0.09, 0.02, and 0.007, respectively). The three groups in this panel show very similar mass distributions to those in the left panel, which also present two distinct peaks at the same mass values. Considering similar mass distributions for different precisions of parameters, all the selected hot subdwarf stars were adopted in the following analysis. + +\begin{figure} + \centering + \includegraphics[width=1\linewidth]{picture/distribute_mass_spclass.pdf} + \caption{Mass distributions for selected hot subdwarf stars with different spectral classifications.} + \label{Fig 6} +\end{figure} +In \Fig \ref{Fig 6}, we present the mass distributions for hot subdwarf stars according to their spectral classifications; for example, He-poor sdB/sdOB (dashed red histogram), He-rich stars (blue histogram, including He-sdB, He-sdO, and He-sdOB), and He-poor sdO (green histogram). The mass distribution of He-poor sdB/sdOB stars, which make up the majority of the hot subdwarf population, closely mirrors that of the entire sample, with two peaks at 0.47 and 0.37 ${\rm M}_{\odot}$. For He-rich hot subdwarfs, two peaks are also present, but the values differ from those seen in sdB/sdOB, occurring at 0.4 and 0.58 ${\rm M}_{\odot}$ (see the discussion in Section 4.3), respectively. However, He-poor sdO stars have a much flatter mass distribution and consist primarily of low-mass stars. + +\section{Discussion} +\subsection{Comparison of mass distribution with previous study} + +We compared the mass distribution of the entire sample with that of \citet{2023ApJLei} in \Fig \ref{Fig 7}. Both mass distributions exhibit a wide mass range of 0.1 - 1.0 ${\rm M}_{\odot}$. This is likely due to the large uncertainties of the input parameters (e.g., parallax and surface gravity) that were used in both studies to estimate the mass of hot subdwarf stars.\LEt{***Verify that your intended meaning has not been changed.} In general, the two mass distributions show a basic consistency in that a primary peak appears around 0.47 ${\rm M}_{\odot}$, and the distribution trend for the low-mass and high-mass sides is nearly the same. As is described in Section 3.3, in addition to the primary one, a second mass peak (around 0.37 ${\rm M}_{\odot}$) is also clearly presented in the mass distribution of this study (red histogram). Nevertheless, this distinct feature is much more obscure in the mass distribution of \citet{2023ApJLei} (dashed blue histogram). Note that the input surface gravities used to calculate mass for the two studies are from different catalogs. The parameters used in this study are from the catalog of \citet{2022A&ACulpan}, which were collected from other literature \citep{2020A&A...635A.193G, 2021ApJS..256...28L, 2021MNRAS.501..623J}. While the parameters used in \citet{2023ApJLei} are from \citet{2018ApJ...868...70L, 2019ApJ...881..135L, 2020ApJ...889..117L, 2023ApJ...942..109L}. The method of spectral analysis and the observed spectra used in these studies could be different, which would lead to the differences in obtained parameters. For example, the systematic errors of surface gravity between \citet{2021ApJS..256...28L} and Lei et al. are around 0.07 dex. Thus, these differences would cause an inconsistency in the mass distribution, especially for some local features. + +\begin{figure} + \centering + \includegraphics[width=1\linewidth]{picture/distribute_mass_with_previos_work.pdf} + \caption{Comparison of mass distribution between this study (red histogram) and \citet{2023ApJLei} (dashed blue histogram).} + \label{Fig 7} +\end{figure} + +\subsection{Mass distribution of He-poor sdB/sdOB stars} + +\citet{2003MNRASHan} (hereafter Han03) have carried out a detailed BPS study on the formation of sdB-type hot subdwarfs. In their study, 12 sets of models were constructed with various input parameters to investigate their impacts on the formation of sdB stars. Among these models, the model of set 2 (with $Z=0.02$, a flat initial mass ratio distribution, $q_{\rm crit}$ = 1.5, $\alpha_{\rm CE}$ = $\alpha_{\rm th}$ = 0.75) was chosen as the best-fitting model in their study, capable of satisfying most of the observed properties for sdB stars. These results from BPS models are highly convenient for making direct comparisons with observations. + +The left panel of \Fig \ref{Fig 8} exhibits comparisons between the mass distribution of set 2 in Han03 (solid black curve) and that of this study (gray histogram). As is discussed in Section 4.1, the mass distribution of sdB/sdOB stars in this study shows a wide range from 0.1 to 1.0 ${\rm M}_{\odot}$ due to the large uncertainties of the surface gravity and parallax, while the mass distribution of Han03 ranges from 0.3 to 0.8 ${\rm M}_{\odot}$, which is narrower than that of this study. Since the minimum core mass for He ignition is about 0.3 ${\rm M}_{\odot}$ (see Table 1 and 2 in \citealt{2002MNRASHan}), there is a cutoff of mass around 0.3 ${\rm M}_{\odot}$ for the low-mass side in the distribution of Han03. Therefore, the stars with masses of less than 0.3 ${\rm M}_{\odot}$ in this study could be low-mass WDs or extremely low-mass (ELM) WDs (also see the discussion in Section 4.4 of \citealt{2023ApJLei}). + +Furthermore, three distinct peaks are presented in the mass distribution of Han03, at around 0.46, 0.4, and 0.36 ${\rm M}_{\odot}$. These were generated through the combination of the first CE, the second CE, and the first stable RLOF channels (see \Fig 12 and Section 7.3 in their study). As can clearly be seen in the panel, the primary mass peak (around 0.47 ${\rm M}_{\odot}$) in our study is consistent very well with the model prediction of Han03. The secondary mass peak in our study (e.g., around 0.36 ${\rm M}_{\odot}$) corresponds to the left mass peak in Han03, which demonstrates that these stars are mainly produced by the stable RLOF channel with their progenitors at the Hertzsprung gap evolution stage. On the other hand, the middle mass peak (e.g., around 0.4 ${\rm M}_{\odot}$) in Han03 is obscure in our mass distribution, for which the stars are mainly produced from the first and the second CE channel with the mass of progenitors around 1.9 ${\rm M}_{\odot}$ (see Table 1 in \citealt{2002MNRASHan}). + + +\begin{figure*} + \centering + \includegraphics[width=0.4\linewidth]{picture/distribute_mass_sdB_sdOB_with_hanset2.pdf} + \includegraphics[width=0.4\linewidth]{picture/distribute_mass_sdB_sdOB_with_segovia2024_all.pdf} + \caption{Left panel: Comparison of mass distribution for sdB/sdOB stars between this study (gray histogram) and Han03 (solid black curve). Right panel: Comparison of mass distribution for sdB/sdOB stars between this study (gray histogram) and \citet{2025PASA...42...12R} (solid black curve).} + \label{Fig 8} +\end{figure*} + +\citet{2025PASA...42...12R} also studied the impacts of various parameters on the formation of sdB stars through BPS methods. Unlike previous BPS models (e.g., Han03, \citealt{2012ApJ...746..186C}), they considered H-rich shells using an analytic prescription in the study that gets more closer to the real evolution of sdB stars. In the right panel of \Fig \ref{Fig 8}, we compare the mass distribution predicted by \citet{2025PASA...42...12R} with that of this study. The mass range of sdB stars predicted by \citet{2025PASA...42...12R} (shown by the solid black curve in the right panel) is roughly from 0.3 to 0.62 ${\rm M}_{\odot}$ and is a little narrower than that of Han03 and this study. Note that the results of two He-WDs merging are not included in the BPS code COMPAS \citep{2022ApJSRiley} that was used in their study\footnote{Although the results of two He-WDs merging are not taken into account in COMPAS, \citet{2025PASA...42...12R} still give a simplified and qualitative analysis on this channel; see Section 3.2.4 in their study and Section 4.3 in this study for details.}; therefore, some massive hot subdwarf stars are absent in the mass distribution of \citet{2025PASA...42...12R}. As is shown in the panel, a sharp primary peak around 0.47 ${\rm M}_{\odot}$ is clearly presented in both two mass distributions, which indicates a good agreement between the predictions of BPS model and observations. Furthermore, a second peak of around 0.37 ${\rm M}_{\odot}$ is also presented in the mass distribution of \citet{2025PASA...42...12R} (see also Fig 7 in \citealt{2025MNRAS.539.3273R}). Although the relative number of stars around this peak in their study is less than that of present study, it shows a one-to-one correspondence between the two studies. + +\subsection{Mass distribution for He-rich Hot subdwarfs} +Two He-WDs merger is considered as the dominant formation channel for He-rich hot subdwarf stars (e.g., $\log(n{\rm He}/n{\rm H})$ $>$ -1.0). The mass range of He-rich hot subdwarfs produced by this channel in Han03 is roughly from 0.42 to 0.76 ${\rm M}_{\odot}$, with a relatively flat peak between 0.5 and 0.6 ${\rm M}_{\odot}$. \citet{2012MNRASZhang} studied three different merging models for two He-WDs, and found that the results could explain most of observed gravities, effective temperatures, and surface chemical abundance for He-rich stars. Furthermore, \citet{2017ApJ...835..242Z} found that the mergers of He-WDs with low-mass MS stars could contribute to the formation of intermediate He-rich (iHe-rich) hot subdwarfs. On the other hand, \citet{2021MNRAS.507.4603M} proposed that MS companions could survive Ia SN explosions and evolve as He-rich hot subdwarfs (see also \citealt{2024RAA....24e5003J}). They obtained a wide mass range of 0.35 to 1.0 ${\rm M}_{\odot}$ for this formation channel, with a mass peak at around 0.4 ${\rm M}_{\odot}$. + +As was mentioned above, \citet{2023ApJLei} obtained a wide mass range and a sharp mass peak around 0.42 ${\rm M}_{\odot}$ for He-rich hot subdwarf stars observed by LAMOST. The mass peak in their study is much lower than the prediction of Han03 and \citet{2012MNRASZhang}. On the other hand, the mass peak in \citet{2023ApJLei} is basically consistent with the value predicted by \citet{2021MNRAS.507.4603M}, but the birth rate for this channel could be too low to explain the discovered He-rich hot subdwarfs (see Section 4.1 of \citealt{2021MNRAS.507.4603M}). According to these results, \citet{2023ApJLei} proposed that, besides the two He-WDs merger, some other channels could contribute to the formation of He-rich hot subdwarfs. \citet{2024ApJS..271...21L} came to a similar conclusion after analyzing the surface chemical abundances of He-rich hot subdwarf stars. + +\begin{figure*} + \centering + \includegraphics[width=1\linewidth]{picture/distribute_mass_He_rich.pdf} + \caption{Left panel: Comparison of mass distribution for He-rich stars between this study (gray histogram) and \citet{2023ApJLei} (dotted red curve). Middle panel: Comparison of mass distribution for He-rich stars between this study and Han03 (solid black curve). Right panel: Comparison of mass distribution for He-rich stars between this study and \citet{2025PASA...42...12R} (dash-dotted blue curve). } + \label{Fig 9} +\end{figure*} + +However, due to the limited size of the sample analyzed in \citet{2023ApJLei}, for example only 39 He-rich stars in group 3 of their sample (see Table 2 in their study), it would influence the statistical results for mass distribution without completeness of sample.\LEt{***Unclear what "it" is referring to here.} Thanks to the deep learning model SENN designed in the present study (see Section 2.1), more than 2000 synthetic SEDs of the selected hot subdwarfs were calculated. Using these information, the masses of 131 He-rich stars were determined in this study, with the sample size being much larger than that analyzed in \citet{2023ApJLei}. Therefore, a comparison of the mass distribution between this study and previous studies could help us better understand the formation of He-rich hot subdwarf stars. + +In the left panel of \Fig \ref{Fig 9}, we compare the mass distribution of He-rich stars obtained in the present study with that of in \citet{2023ApJLei}. As can be seen in the panel, it exhibits a relatively wide mass distribution that is roughly from 0.3 to 0.9 ${\rm M}_{\odot}$ for both two studies (Note that hot subdwarf stars with masses of less than 0.3 ${\rm M}_{\odot}$ cannot be produced in model predictions; thus, we excluded these stars from our results for the comparison).\LEt{***Verify that your intended meaning has not been changed.} Two distinct mass peaks are presented in the mass distribution of this study (gray histogram): a primary peak around 0.56 ${\rm M}_{\odot}$ and a secondary peak around 0.4 ${\rm M}_{\odot}$. As was mentioned above, a sharp mass peak around 0.42 ${\rm M}_{\odot}$ is clearly shown in the mass distribution of \citet{2023ApJLei} (dotted red curve), which corresponds to the secondary mass peak in this study. However, it could be due to the small sample size used in the study of \citet{2023ApJLei} that no distinct mass peak between 0.5 and 0.6 ${\rm M}_{\odot}$ can be distinguished in their mass distribution.\LEt{***Verify that your intended meaning has not been changed.} + +In the middle panel of \Fig \ref{Fig 9}, we compare the mass distribution of He-rich stars in this study with that of Han03. As can be seen clearly in the panel, our mass distribution is much wider than that in Han03 (e.g., roughly from 0.42 to 0.76 ${\rm M}_{\odot}$, solid black curve). As was discussed in Section 4.1, this could be due to the large uncertainties of the parallax and gravity, which significantly affect the precision of mass determination in this study. He-rich stars produced through two He-WDs merger in Han03 present a flat mass peak between 0.5 and 0.6 ${\rm M}_{\odot}$, which could corresponding roughly to the primary mass peak around 0.56 ${\rm M}_{\odot}$ in this study. However, the secondary mass peak around 0.4 ${\rm M}_{\odot}$ is not predicted by BPS models of Han03, which would demonstrate that two He-WDs merging channel cannot explain the formation of all He-rich hot subdwarf stars. + +Nevertheless, it leads to a little different conclusion when comparing our results with recent BPS model predictions from \citet{2025PASA...42...12R} (see the right panel in \Fig \ref{Fig 9}).\LEt{***Unclear what "it" is referring to here.} The mass distribution of He-rich stars from the merging channel of \citet{2025PASA...42...12R} (dash-dotted blue curve) presents two distinct mass peaks around 0.55 ${\rm M}_{\odot}$ and 0.41 ${\rm M}_{\odot}$ (see \Fig 14 in their study), which correspond perfectly to the two peaks shown in our study (gray histogram). However, the relative number of He-rich stars around the secondary mass peak (e.g., 0.41 ${\rm M}_{\odot}$) predicted by \citet{2025PASA...42...12R} is less than in this study. As is discussed in Section 3.2.4 of their study, the secondary mass peak heavily depends on mass-transfer accretion efficiency at stable RLOF phase. It would disappear when the accretion efficiency equals 0, and it would merge with the primary peak and form a symmetrical distribution with a peak around 0.47 ${\rm M}_{\odot}$ if the accretion efficiency equals 1. + + Note that the formation of two He-WD binaries\footnote{In \citet{2025PASA...42...12R}, the treatment of the two He-WDs' merging channel was very sample. They did not evolve the two He-WDs binary into merging phase, but instead considered the binary system as hot subdwarfs if they could merge within the age of our Universe (e.g., 14 Gyr).\LEt{***Verify that your intended meaning has not been changed.}} requires two RLOF phases. The whole envelope of the primary star will be removed through stable mass transfer during the first RLOF phase, while the two components will be surrounded by a CE formed due to unstable mass transfer during the second RLOF phase, and the CE should be ejected before the two He-WDs binary is formed \citep{1984ApJ...277..355W}. The mass-transfer accretion efficiency during the first RLOF phase has significant effects on the loss of angular momentum due to mass loss from the system, which in turn determines the subsequent evolution of the orbital separation. Therefore, a lower accretion efficiency during the first RLOF phase would result in either systems not triggering CE events (too far from each other) or merging (too close), both resulting in a final configuration different from the two He-WD binaries. \LEt{***Verify that your intended meaning has not been changed.} + + Based on the discussion mentioned above, if the second mass peak (around 0.4 ${\rm M}_{\odot}$) is a real feature, the two He-WDs merging channel could produce most of the observed He-rich hot subdwarf stars on the condition that mass transfer during the first RLOF phase to produce the two He-WDs' binary should be partially conserved, and the accretion efficiency is not too low.\LEt{***Verify that your intended meaning has not been changed. Single-sentence paragraphs should be avoided.} + +\section{Summary} + +In this study, a deep learning model SENN was designed to calculate synthetic SEDs for a large number of known hot subdwarfs with the help of spectra from LAMOST and SDSS. Through the VOSA service of the Spanish Virtual Observatory, the physical parameters (e.g., masses, radii, and luminosities) of 1,012 hot subdwarfs were obtained by comparing the synthetic SEDs with the observed flux density. With the obtained parameters for a large sample size, comparisons between observations and model predictions would help us understand the formation of hot subdwarf stars more deeply and comprehensively. + +The two mass peaks (e.g., 0.47 and 0.37) in the mass distribution of sdB/sdOB stars are consistent with the prediction from BPS models, which corresponds to the production of CE ejection and stable RLOF respectively. There is also a primary peak (around 0.56 ${\rm M}_{\odot}$) and a secondary peak (around 0.4 ${\rm M}_{\odot}$) clearly visible in the mass distribution of He-rich stars. Although the primary mass peak is well predicted by BPS models, the occurrence of the secondary peak in the models depends heavily on the mass-transfer accretion efficiency at stable RLOF stage in binary evolution. These results indicate that the two He-WDs' merging channel could produce most of the observed He-rich hot subdwarf stars, but mass transfer should be partially conserved during the stable RLOF phase.\LEt{***Verify that your intended meaning has not been changed.} Considering the large uncertainties of the masses obtained in this study, other alternative formation channels for He-rich hot subdwarfs would not be completely excluded. More accurate determinations of the physical parameters of hot subdwarf stars are urgently needed. + +It is important to note that although we could efficiently obtain synthetic SEDs of hot subdwarfs using the SENN model, deriving their masses, radii, and luminosities still requires atmospheric parameters ($T_{\text{eff}}$ and ${\rm log} g$). Accurate atmospheric parameters, however, must still be acquired through the conventional method of synthetic spectral fitting.‌ + +Fortunately, we are actively exploring the use of machine learning methods to predict the atmospheric parameters of hot subdwarfs \citep{2026ApJS..283...16L}. This approach, in the near future, should enable us to directly obtain both the atmospheric parameters and masses of hot subdwarfs using artificial intelligence techniques, without having to compute stellar atmosphere models. + +\section{Data availability} + +Table \ref{tab1} is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/. + +\begin{acknowledgements} + + We greatly thank the referee for his/her valuable comments and useful suggestions, which help improve the manuscript significantly. We also thank Nicolás Rodríguez-Segovia for his detailed suggestions on the discussion of Section 4.3. +This work acknowledges support from the National Natural Science Foundation of China (Nos. 12073020, 12588202 and 12273055), Scientific Research Fund of Hunan Provincial Education Department + grant No. 20K124 and 23A0132, the Strategic Priority Research Program of Chinese Academy of Sciences, grant No. XDB1160301. K.H. acknowledges support from the Scientific Research Funds of Hunan Provincial Education Department (Nos. 22A0099 and 24A0101). + This research has made use of the Spanish Virtual Observatory (\url{https://svo.cab.inta-csic.es}) project funded by MCIN/AEI/10.13039/501100011025/ through grant PID2020-112949GB-I00. Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences. +\end{acknowledgements} + +\bibliography{bib} +\bibliographystyle{aa} +\begin{appendix} +\onecolumn +\section{Main parameters for the selected hot subdwarf stars} +\begin{table}[!ht] + \centering + \caption{Main parameters for part of 1,012 selected hot subdwarf stars} + {\fontsize{6}{10}\selectfont + \setlength{\tabcolsep}{2pt} + \begin{tabular}{lllllllllll} + \hline + \centering + Name & \multicolumn{1}{c}{Source\_id} & \multicolumn{1}{c}{sp\_class} & \multicolumn{1}{c}{$T_{\rm eff}$} & \multicolumn{1}{c}{${\rm log} g$} & \multicolumn{1}{c}{$A_{\rm V}$} & \multicolumn{1}{c}{plx\_zp } & \multicolumn{1}{c}{Angular diameter} & \multicolumn{1}{c}{Radius} & \multicolumn{1}{c}{Luminosity} & \multicolumn{1}{c}{Mass} \\ + \multicolumn{1}{c}{} & \multicolumn{1}{c}{Gaia DR3} & \multicolumn{1}{c}{} & \multicolumn{1}{c}{K} & \multicolumn{1}{c}{(cm\ s$^{-2}$)} & \multicolumn{1}{c}{mag} & \multicolumn{1}{c}{mas} & \multicolumn{1}{c}{log(rad)} & \multicolumn{1}{c}{R/R$_{\odot}$} & \multicolumn{1}{c}{L/L$_{\odot}$} & \multicolumn{1}{c}{M/M$_{\odot}$} \\ + \hline + BD+423250 & 2105469320138052864 & sdB & $28700\pm1000$ & $5.08\pm0.02$ & 0.422 & $4.1508\pm0.0319$ & $-10.268^{+0.036}_{-0.020}$ & $0.287^{+0.003}_{-0.003}$ & $50.2^{+7.5}_{-6.8}$ & $0.36^{+0.03}_{-0.03}$ \\ +BD+481777 & 825628714431805056 & sdO & $47565\pm251$ & $5.84\pm0.04$ & 0.010 & $4.2560\pm0.0617$ & $-10.503^{+0.019}_{-0.014}$ & $0.163^{+0.003}_{-0.003}$ & $122.7^{+4.7}_{-4.5}$ & $0.67^{+0.07}_{-0.07}$ \\ +BD-32179 & 3068744791442939904 & sdO & $59121\pm686$ & $4.55\pm0.03$ & 0.010 & $1.0124\pm0.0666$ & $-10.458^{+0.020}_{-0.029}$ & $0.767^{+0.054}_{-0.047}$ & $6445.7^{+992.0}_{-811.9}$ & $0.76^{+0.13}_{-0.10}$ \\ +BPSCS22890-74 & 4420741294390728448 & sdB & $24560\pm567$ & $5.14\pm0.06$ & 1.135 & $1.0170\pm0.0312$ & $-10.690^{+0.064}_{-0.016}$ & $0.430^{+0.014}_{-0.013}$ & $60.4^{+7.1}_{-6.4}$ & $0.93^{+0.15}_{-0.13}$ \\ +Bal90100005 & 2845710850610464640 & sdB & $32789\pm123$ & $5.66\pm0.02$ & 0.302 & $1.2124\pm0.0358$ & $-11.098^{+0.011}_{-0.052}$ & $0.146^{+0.005}_{-0.005}$ & $22.2^{+2.0}_{-1.9}$ & $0.36^{+0.04}_{-0.03}$ \\ +Bal90900004 & 1874534323107953664 & sdB & $42860\pm1590$ & $5.51\pm0.12$ & 0.168 & $1.3991\pm0.0553$ & $-10.883^{+0.018}_{-0.016}$ & $0.207^{+0.009}_{-0.008}$ & $129.9^{+23.4}_{-20.3}$ & $0.51^{+0.17}_{-0.13}$ \\ +CBS250 & 1373881186687373696 & sdB & $32280\pm140$ & $5.76\pm0.03$ & 0.052 & $0.8909\pm0.0328$ & $-11.194^{+0.010}_{-0.007}$ & $0.159^{+0.006}_{-0.006}$ & $24.6^{+2.4}_{-2.2}$ & $0.53^{+0.06}_{-0.05}$ \\ +CBS274 & 1605239049014274560 & sdOB & $36833\pm2000$ & $5.83\pm0.20$ & 0.030 & $0.3374\pm0.0601$ & $-11.708^{+0.014}_{-0.005}$ & $0.128^{+0.028}_{-0.020}$ & $27.3^{+15.3}_{-9.1}$ & $0.41^{+0.34}_{-0.18}$ \\ +CBS282 & 1591755325606144640 & sdOB & $36728\pm932$ & $6.02\pm0.14$ & 0.457 & $0.3160\pm0.0622$ & $-11.696^{+0.024}_{-0.010}$ & $0.139^{+0.034}_{-0.023}$ & $31.5^{+17.6}_{-9.9}$ & $0.75^{+0.53}_{-0.29}$ \\ +CBS374 & 1471988375850922368 & sdOB & $35110\pm73$ & $6.08\pm0.02$ & 0.093 & $1.0166\pm0.0376$ & $-11.195^{+0.025}_{-0.006}$ & $0.139^{+0.006}_{-0.005}$ & $26.3^{+2.5}_{-2.3}$ & $0.85^{+0.08}_{-0.07}$ \\ +CBS98 & 810691780249660800 & sdOB & $33588\pm147$ & $5.39\pm0.03$ & 0.029 & $0.6313\pm0.0665$ & $-11.408^{+0.015}_{-0.008}$ & $0.136^{+0.016}_{-0.013}$ & $21.0^{+5.4}_{-4.1}$ & $0.16^{+0.05}_{-0.04}$ \\ +EGGR113 & 4422600328035803264 & sdO & $61075\pm1182$ & $5.77\pm0.05$ & 0.146 & $0.7145\pm0.0416$ & $-11.398^{+0.005}_{-0.034}$ & $0.124^{+0.008}_{-0.007}$ & $192.9^{+29.2}_{-24.8}$ & $0.33^{+0.06}_{-0.05}$ \\ +FBS0021+418 & 382086995098288896 & sdB & $29032\pm477$ & $5.12\pm0.06$ & 0.224 & $0.3996\pm0.0475$ & $-11.341^{+0.013}_{-0.004}$ & $0.252^{+0.034}_{-0.027}$ & $40.7^{+12.1}_{-8.6}$ & $0.31^{+0.10}_{-0.07}$ \\ +FBS0033+376 & 368263110278860544 & sdB & $38970\pm1330$ & $5.89\pm0.10$ & 0.076 & $1.4164\pm0.0409$ & $-11.144^{+0.008}_{-0.006}$ & $0.112^{+0.004}_{-0.004}$ & $26.2^{+4.3}_{-3.9}$ & $0.36^{+0.10}_{-0.08}$ \\ +FBS0051+377 & 364742852004132736 & sdOB & $35103\pm116$ & $5.91\pm0.02$ & 0.080 & $1.0341\pm0.0418$ & $-11.181^{+0.018}_{-0.006}$ & $0.142^{+0.006}_{-0.006}$ & $27.3^{+2.8}_{-2.5}$ & $0.59^{+0.06}_{-0.06}$ \\ +FBS0102+362 & 369576820516013824 & sdB & $32628\pm98$ & $5.68\pm0.02$ & 0.011 & $2.6839\pm0.0523$ & $-10.729^{+0.007}_{-0.007}$ & $0.154^{+0.004}_{-0.004}$ & $24.1^{+1.7}_{-1.7}$ & $0.41^{+0.03}_{-0.03}$ \\ +FBS0104+367 & 369621277722573568 & sdB & $31086\pm120$ & $5.94\pm0.04$ & 0.157 & $0.7730\pm0.0421$ & $-11.236^{+0.044}_{-0.008}$ & $0.166^{+0.010}_{-0.009}$ & $23.0^{+3.1}_{-2.7}$ & $0.87^{+0.14}_{-0.12}$ \\ +FBS0106+374 & 369573831218501376 & sdB & $30340\pm218$ & $5.75\pm0.05$ & 0.141 & $1.1993\pm0.0391$ & $-10.953^{+0.005}_{-0.006}$ & $0.207^{+0.007}_{-0.007}$ & $32.6^{+2.8}_{-2.6}$ & $0.88^{+0.13}_{-0.11}$ \\ +FBS0117+396 & 371711041304831616 & sdB & $28500\pm100$ & $5.42\pm0.01$ & 0.060 & $0.5853\pm0.0462$ & $-11.279^{+0.035}_{-0.007}$ & $0.198^{+0.017}_{-0.014}$ & $23.3^{+4.4}_{-3.5}$ & $0.38^{+0.07}_{-0.06}$ \\ +FBS0156+439 & 346721341030064640 & He-sdOB & $43970\pm1190$ & $5.72\pm0.16$ & 0.166 & $0.5015\pm0.0491$ & $-11.401^{+0.031}_{-0.009}$ & $0.176^{+0.019}_{-0.016}$ & $103.6^{+26.9}_{-20.1}$ & $0.59^{+0.31}_{-0.20}$ \\ +FBS0203+374 & 330722897089067392 & sdB & $28744\pm303$ & $5.47\pm0.04$ & 0.150 & $1.0701\pm0.0367$ & $-10.984^{+0.044}_{-0.004}$ & $0.214^{+0.008}_{-0.007}$ & $28.0^{+2.7}_{-2.6}$ & $0.49^{+0.06}_{-0.06}$ \\ +FBS0206+428 & 351633546665907200 & sdB & $25735\pm251$ & $5.14\pm0.03$ & 0.135 & $0.9280\pm0.0366$ & $-11.019^{+0.006}_{-0.007}$ & $0.229^{+0.009}_{-0.009}$ & $20.6^{+2.4}_{-2.2}$ & $0.26^{+0.04}_{-0.03}$ \\ +FBS0208+390 & 332606704106366848 & sdB & $38743\pm269$ & $6.15\pm0.04$ & 0.106 & $0.7313\pm0.0419$ & $-11.439^{+0.008}_{-0.011}$ & $0.111^{+0.007}_{-0.006}$ & $24.8^{+3.5}_{-3.0}$ & $0.63^{+0.10}_{-0.09}$ \\ +FBS0212+334 & 326009496898928896 & sdB & $29697\pm197$ & $5.63\pm0.04$ & 0.254 & $1.2116\pm0.0350$ & $-10.875^{+0.012}_{-0.006}$ & $0.243^{+0.007}_{-0.007}$ & $41.3^{+3.0}_{-2.9}$ & $0.92^{+0.11}_{-0.10}$ \\ +FBS0314+372 & 235323736345986176 & sdB & $29283\pm192$ & $5.42\pm0.03$ & 0.902 & $0.8740\pm0.0403$ & $-11.085^{+0.007}_{-0.029}$ & $0.209^{+0.010}_{-0.009}$ & $28.8^{+3.3}_{-2.9}$ & $0.42^{+0.06}_{-0.05}$ \\ +FBS0324+379 & 234861632224343424 & sdB & $24809\pm298$ & $5.27\pm0.03$ & 0.473 & $1.3008\pm0.0340$ & $-10.908^{+0.009}_{-0.007}$ & $0.210^{+0.006}_{-0.006}$ & $15.0^{+1.8}_{-1.7}$ & $0.30^{+0.03}_{-0.03}$ \\ +FBS0638+428 & 963881581386403072 & sdB & $28090\pm161$ & $5.29\pm0.02$ & 0.229 & $1.1992\pm0.0344$ & $-10.985^{+0.042}_{-0.010}$ & $0.191^{+0.006}_{-0.006}$ & $20.4^{+1.9}_{-1.9}$ & $0.26^{+0.03}_{-0.03}$ \\ +FBS0639+391 & 944892878136403712 & sdB & $29658\pm509$ & $5.53\pm0.08$ & 0.372 & $0.8262\pm0.0358$ & $-11.070^{+0.008}_{-0.007}$ & $0.229^{+0.010}_{-0.010}$ & $36.3^{+4.5}_{-4.0}$ & $0.65^{+0.15}_{-0.12}$ \\ +FBS0646+386 & 944390774983674496 & sdB & $33238\pm190$ & $5.63\pm0.03$ & 0.234 & $0.7018\pm0.0473$ & $-11.323^{+0.020}_{-0.012}$ & $0.150^{+0.011}_{-0.010}$ & $24.6^{+3.9}_{-3.4}$ & $0.35^{+0.06}_{-0.05}$ \\ +FBS1400+389 & 1495942160078351744 & sdOB & $18800\pm1000$ & $4.71\pm0.10$ & 0.029 & $1.4515\pm0.0345$ & $-10.534^{+0.020}_{-0.045}$ & $0.449^{+0.011}_{-0.011}$ & $22.6^{+5.5}_{-4.7}$ & $0.38^{+0.10}_{-0.08}$ \\ +FBS1531+381 & 1375814952762454272 & sdB & $29230\pm125$ & $5.58\pm0.03$ & 0.029 & $1.9294\pm0.0345$ & $-10.805^{+0.013}_{-0.164}$ & $0.181^{+0.004}_{-0.004}$ & $21.5^{+1.7}_{-1.6}$ & $0.46^{+0.04}_{-0.04}$ \\ +FBS1715+424 & 1360139937040515072 & sdO & $58438\pm514$ & $6.11\pm0.03$ & 0.010 & $2.3950\pm0.0387$ & $-10.911^{+0.011}_{-0.009}$ & $0.114^{+0.003}_{-0.003}$ & $135.4^{+6.8}_{-6.4}$ & $0.61^{+0.05}_{-0.05}$ \\ +FBS1745+437 & 1349088676950060672 & sdB & $33601\pm109$ & $5.56\pm0.02$ & 0.073 & $1.0659\pm0.0262$ & $-11.132^{+0.008}_{-0.006}$ & $0.153^{+0.004}_{-0.004}$ & $26.9^{+2.0}_{-1.9}$ & $0.31^{+0.03}_{-0.03}$ \\ +FBS2255+404 & 1930945626165804032 & He-sdOB & $48127\pm277$ & $5.92\pm0.04$ & 0.355 & $0.4056\pm0.0444$ & $-11.490^{+0.049}_{-0.010}$ & $0.176^{+0.022}_{-0.017}$ & $149.9^{+39.4}_{-28.1}$ & $0.95^{+0.27}_{-0.19}$ \\ +FBS2307+338 & 1911572540520290048 & He-sdO & $50664\pm390$ & $5.85\pm0.04$ & 0.219 & $0.4957\pm0.0502$ & $-11.435^{+0.006}_{-0.011}$ & $0.165^{+0.018}_{-0.015}$ & $160.2^{+38.3}_{-28.2}$ & $0.70^{+0.18}_{-0.14}$ \\ +FBS2347+385 & 2881551562420806784 & sdB & $23770\pm350$ & $5.38\pm0.06$ & 0.269 & $3.9390\pm0.0341$ & $-10.434^{+0.026}_{-0.011}$ & $0.207^{+0.003}_{-0.003}$ & $12.3^{+1.6}_{-1.6}$ & $0.37^{+0.06}_{-0.05}$ \\ +Feige114 & 1858674589447492608 & sdOB & $37689\pm189$ & $5.56\pm0.02$ & 0.148 & $1.2354\pm0.0317$ & $-10.983^{+0.023}_{-0.006}$ & $0.186^{+0.005}_{-0.005}$ & $62.5^{+3.8}_{-3.6}$ & $0.46^{+0.04}_{-0.04}$ \\ +Feige26 & 2503706418759709184 & He-sdO & $65608\pm912$ & $5.46\pm0.04$ & 0.010 & $0.5763\pm0.0471$ & $-11.247^{+0.007}_{-0.010}$ & $0.218^{+0.019}_{-0.017}$ & $793.7^{+154.1}_{-121.7}$ & $0.50^{+0.11}_{-0.09}$ \\ +Feige34 & 781164326766404736 & sdO & $62400\pm330$ & $5.95\pm0.02$ & 0.145 & $4.4105\pm0.1039$ & $-10.645^{+0.069}_{-0.018}$ & $0.113^{+0.003}_{-0.003}$ & $174.4^{+9.3}_{-8.8}$ & $0.42^{+0.04}_{-0.03}$ \\ +Feige67 & 3935488605023787392 & sdO & $61114\pm318$ & $5.92\pm0.01$ & 0.105 & $2.9833\pm0.0735$ & $-10.739^{+0.010}_{-0.039}$ & $0.136^{+0.004}_{-0.004}$ & $232.9^{+13.0}_{-12.0}$ & $0.56^{+0.04}_{-0.04}$ \\ +GALEXJ00468+1956 & 2801277176253968640 & sdB & $32891\pm111$ & $5.84\pm0.02$ & 0.200 & $0.9281\pm0.0413$ & $-11.213^{+0.041}_{-0.008}$ & $0.146^{+0.007}_{-0.006}$ & $22.2^{+2.5}_{-2.3}$ & $0.53^{+0.06}_{-0.05}$ \\ +GALEXJ00476+3123 & 360511037906831872 & sdB & $31069\pm166$ & $5.65\pm0.03$ & 0.207 & $1.0593\pm0.0383$ & $-11.149^{+0.042}_{-0.011}$ & $0.148^{+0.006}_{-0.006}$ & $18.4^{+2.0}_{-1.9}$ & $0.36^{+0.04}_{-0.04}$ \\ +GALEXJ00498+3522 & 363795760175504768 & sdOB & $36551\pm243$ & $5.74\pm0.04$ & 0.063 & $0.8767\pm0.0412$ & $-11.251^{+0.010}_{-0.016}$ & $0.142^{+0.007}_{-0.007}$ & $32.5^{+3.7}_{-3.3}$ & $0.41^{+0.06}_{-0.05}$ \\ +GALEXJ01012+3125 & 312628749626419328 & sdB & $28202\pm155$ & $5.45\pm0.02$ & 0.063 & $1.8070\pm0.0362$ & $-10.788^{+0.010}_{-0.017}$ & $0.201^{+0.005}_{-0.004}$ & $22.9^{+1.8}_{-1.7}$ & $0.41^{+0.03}_{-0.03}$ \\ +GALEXJ01194+4901 & 400211958948711552 & He-sdOB & $43720\pm510$ & $5.86\pm0.21$ & 0.313 & $1.2614\pm0.0326$ & $-10.965^{+0.017}_{-0.012}$ & $0.189^{+0.005}_{-0.005}$ & $117.7^{+8.6}_{-8.0}$ & $0.95^{+0.59}_{-0.37}$ \\ +GALEXJ01509+3107 & 304311150320629376 & sdB & $30183\pm189$ & $5.84\pm0.04$ & 0.130 & $1.3955\pm0.0367$ & $-11.041^{+0.004}_{-0.008}$ & $0.145^{+0.004}_{-0.004}$ & $15.6^{+1.7}_{-1.7}$ & $0.53^{+0.06}_{-0.06}$ \\ +GALEXJ01543+4905 & 357580873780641920 & sdB & $32100\pm410$ & $5.50\pm0.32$ & 0.452 & $1.7860\pm0.0250$ & $-10.871^{+0.008}_{-0.008}$ & $0.166^{+0.003}_{-0.003}$ & $26.4^{+2.1}_{-2.1}$ & $0.32^{+0.35}_{-0.17}$ \\ +GALEXJ02069+1438 & 77515058657678592 & sdB & $30310\pm660$ & $5.77\pm0.06$ & 0.132 & $2.2104\pm0.0447$ & $-10.881^{+0.010}_{-0.028}$ & $0.133^{+0.003}_{-0.003}$ & $13.3^{+1.9}_{-1.9}$ & $0.38^{+0.06}_{-0.05}$ \\ +GALEXJ02163+2759 & 107585292928397568 & sdB & $25480\pm450$ & $5.35\pm0.05$ & 0.155 & $1.5540\pm0.0313$ & $-10.767^{+0.028}_{-0.013}$ & $0.244^{+0.005}_{-0.005}$ & $22.5^{+2.4}_{-2.3}$ & $0.49^{+0.07}_{-0.06}$ \\ +GALEXJ02328+4411 & 341195058150383104 & sdB & $33260\pm420$ & $5.73\pm0.10$ & 0.237 & $1.2611\pm0.0577$ & $-11.082^{+0.011}_{-0.007}$ & $0.145^{+0.007}_{-0.007}$ & $23.1^{+2.9}_{-2.7}$ & $0.41^{+0.12}_{-0.09}$ \\ +GALEXJ04158+0154 & 3259060049366022400 & sdBV & $34773\pm123$ & $5.79\pm0.02$ & 0.359 & $1.5335\pm0.0402$ & $-11.003^{+0.014}_{-0.006}$ & $0.144^{+0.004}_{-0.004}$ & $27.1^{+2.1}_{-2.0}$ & $0.46^{+0.04}_{-0.04}$ \\ +GALEXJ04205+0120 & 3255780171819962496 & He-sdO & $46050\pm910$ & $5.97\pm0.16$ & 0.081 & $2.4658\pm0.0620$ & $-10.816^{+0.012}_{-0.006}$ & $0.137^{+0.004}_{-0.004}$ & $76.2^{+7.5}_{-6.9}$ & $0.64^{+0.29}_{-0.20}$ \\ +GALEXJ04593-0228 & 3225359193340812288 & sdB & $30613\pm608$ & $5.70\pm0.12$ & 0.062 & $1.1390\pm0.0412$ & $-11.197^{+0.033}_{-0.008}$ & $0.124^{+0.005}_{-0.005}$ & $12.0^{+2.0}_{-1.9}$ & $0.28^{+0.09}_{-0.07}$ \\ +GALEXJ05369+3955 & 190970433715259904 & He-sdOB & $38898\pm169$ & $5.79\pm0.04$ & 0.507 & $1.3436\pm0.0332$ & $-11.007^{+0.006}_{-0.008}$ & $0.164^{+0.005}_{-0.004}$ & $55.1^{+3.3}_{-3.1}$ & $0.60^{+0.07}_{-0.06}$ \\ +GALEXJ05557+6408 & 287018271958898560 & sdO & $45600\pm3380$ & $5.73\pm0.39$ & 0.462 & $1.9389\pm0.0248$ & $-10.932^{+0.007}_{-0.023}$ & $0.134^{+0.003}_{-0.003}$ & $70.1^{+23.2}_{-18.7}$ & $0.35^{+0.51}_{-0.21}$ \\ +GALEXJ06134+3420 & 3452237404778065152 & sdOB & $34250\pm390$ & $5.75\pm0.10$ & 0.432 & $1.7373\pm0.0329$ & $-10.935^{+0.010}_{-0.010}$ & $0.148^{+0.003}_{-0.003}$ & $27.1^{+2.2}_{-2.1}$ & $0.45^{+0.12}_{-0.10}$ \\ +GALEXJ063952.00+515658.00 & 992534888766785024 & sdB & $30400\pm340$ & $5.58\pm0.13$ & 0.065 & $3.0845\pm0.0455$ & $-10.552^{+0.031}_{-0.006}$ & $0.202^{+0.004}_{-0.004}$ & $31.2^{+2.2}_{-2.1}$ & $0.56^{+0.20}_{-0.15}$ \\ +GALEXJ06437+3201 & 937248901501446272 & sdB & $26956\pm303$ & $5.12\pm0.04$ & 0.331 & $1.0644\pm0.0448$ & $-10.873^{+0.061}_{-0.008}$ & $0.276^{+0.012}_{-0.011}$ & $36.0^{+3.9}_{-3.5}$ & $0.37^{+0.05}_{-0.05}$ \\ +GALEXJ06463+2920 & 3386622158606040960 & sdOB & $41489\pm229$ & $6.16\pm0.03$ & 0.073 & $2.1178\pm0.0437$ & $-10.998^{+0.009}_{-0.016}$ & $0.105^{+0.003}_{-0.003}$ & $29.3^{+2.0}_{-1.9}$ & $0.58^{+0.05}_{-0.05}$ \\ +GALEXJ07013+5329 & 981727582818800128 & He-sdO & $67230\pm3880$ & $5.60\pm0.22$ & 0.117 & $0.3925\pm0.0431$ & $-11.375^{+0.012}_{-0.005}$ & $0.238^{+0.029}_{-0.023}$ & $1038.8^{+393.0}_{-282.0}$ & $0.83^{+0.61}_{-0.35}$ \\ +GALEXJ07104+2333 & 3368383116127317120 & sdB & $55420\pm24300$ & $5.21\pm0.43$ & 0.724 & $0.5599\pm0.0242$ & $-11.119^{+0.071}_{-0.016}$ & $0.299^{+0.013}_{-0.013}$ & $756.7^{+2464.1}_{-679.2}$ & $0.53^{+0.90}_{-0.33}$ \\ +GALEXJ07108+5624 & 988436459174352512 & sdB & $39970\pm980$ & $5.91\pm0.14$ & 0.094 & $0.9733\pm0.0521$ & $-11.251^{+0.009}_{-0.005}$ & $0.128^{+0.007}_{-0.007}$ & $37.5^{+6.1}_{-5.2}$ & $0.49^{+0.20}_{-0.14}$ \\ +GALEXJ07248+1923 & 3362730178953977472 & sdB & $25777\pm334$ & $5.25\pm0.03$ & 0.172 & $0.9219\pm0.0378$ & $-11.069^{+0.010}_{-0.006}$ & $0.205^{+0.009}_{-0.008}$ & $16.7^{+2.2}_{-2.1}$ & $0.27^{+0.04}_{-0.04}$ \\ + \hline + \end{tabular}} + \label{tab1} +\end{table} + +\end{appendix} +\end{document} diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa54562-25_rev.4/table1.dat b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa54562-25_rev.4/table1.dat new file mode 100644 index 0000000..bdfce7f --- /dev/null +++ b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aa54562-25_rev.4/table1.dat @@ -0,0 +1,1012 @@ +BD+423250 2105469320138052864 sdB 28700 1000 5.08 0.02 0.422 4.1508 0.0319 -10.268 0.036 0.020 0.287 0.003 0.003 50.2 7.5 6.8 0.36 0.03 0.03 +BD+481777 825628714431805056 sdO 47565 251 5.84 0.04 0.010 4.2560 0.0617 -10.503 0.019 0.014 0.163 0.003 0.003 122.7 4.7 4.5 0.67 0.07 0.07 +BD-32179 3068744791442939904 sdO 59121 686 4.55 0.03 0.010 1.0124 0.0666 -10.458 0.020 0.029 0.767 0.054 0.047 6445.7 992.0 811.9 0.76 0.13 0.10 +BPSCS22890-74 4420741294390728448 sdB 24560 567 5.14 0.06 1.135 1.0170 0.0312 -10.690 0.064 0.016 0.430 0.014 0.013 60.4 7.1 6.4 0.93 0.15 0.13 +Bal90100005 2845710850610464640 sdB 32789 123 5.66 0.02 0.302 1.2124 0.0358 -11.098 0.011 0.052 0.146 0.005 0.005 22.2 2.0 1.9 0.36 0.04 0.03 +Bal90900004 1874534323107953664 sdB 42860 1590 5.51 0.12 0.168 1.3991 0.0553 -10.883 0.018 0.016 0.207 0.009 0.008 129.9 23.4 20.3 0.51 0.17 0.13 +CBS250 1373881186687373696 sdB 32280 140 5.76 0.03 0.052 0.8909 0.0328 -11.194 0.010 0.007 0.159 0.006 0.006 24.6 2.4 2.2 0.53 0.06 0.05 +CBS274 1605239049014274560 sdOB 36833 2000 5.83 0.20 0.030 0.3374 0.0601 -11.708 0.014 0.005 0.128 0.028 0.020 27.3 15.3 9.1 0.41 0.34 0.18 +CBS282 1591755325606144640 sdOB 36728 932 6.02 0.14 0.457 0.3160 0.0622 -11.696 0.024 0.010 0.139 0.034 0.023 31.5 17.6 9.9 0.75 0.53 0.29 +CBS374 1471988375850922368 sdOB 35110 73 6.08 0.02 0.093 1.0166 0.0376 -11.195 0.025 0.006 0.139 0.006 0.005 26.3 2.5 2.3 0.85 0.08 0.07 +CBS98 810691780249660800 sdOB 33588 147 5.39 0.03 0.029 0.6313 0.0665 -11.408 0.015 0.008 0.136 0.016 0.013 21.0 5.4 4.1 0.16 0.05 0.04 +EGGR113 4422600328035803264 sdO 61075 1182 5.77 0.05 0.146 0.7145 0.0416 -11.398 0.005 0.034 0.124 0.008 0.007 192.9 29.2 24.8 0.33 0.06 0.05 +FBS0021+418 382086995098288896 sdB 29032 477 5.12 0.06 0.224 0.3996 0.0475 -11.341 0.013 0.004 0.252 0.034 0.027 40.7 12.1 8.6 0.31 0.10 0.07 +FBS0033+376 368263110278860544 sdB 38970 1330 5.89 0.10 0.076 1.4164 0.0409 -11.144 0.008 0.006 0.112 0.004 0.004 26.2 4.3 3.9 0.36 0.10 0.08 +FBS0051+377 364742852004132736 sdOB 35103 116 5.91 0.02 0.080 1.0341 0.0418 -11.181 0.018 0.006 0.142 0.006 0.006 27.3 2.8 2.5 0.59 0.06 0.06 +FBS0102+362 369576820516013824 sdB 32628 98 5.68 0.02 0.011 2.6839 0.0523 -10.729 0.007 0.007 0.154 0.004 0.004 24.1 1.7 1.7 0.41 0.03 0.03 +FBS0104+367 369621277722573568 sdB 31086 120 5.94 0.04 0.157 0.7730 0.0421 -11.236 0.044 0.008 0.166 0.010 0.009 23.0 3.1 2.7 0.87 0.14 0.12 +FBS0106+374 369573831218501376 sdB 30340 218 5.75 0.05 0.141 1.1993 0.0391 -10.953 0.005 0.006 0.207 0.007 0.007 32.6 2.8 2.6 0.88 0.13 0.11 +FBS0117+396 371711041304831616 sdB 28500 100 5.42 0.01 0.060 0.5853 0.0462 -11.279 0.035 0.007 0.198 0.017 0.014 23.3 4.4 3.5 0.38 0.07 0.06 +FBS0156+439 346721341030064640 He-sdOB 43970 1190 5.72 0.16 0.166 0.5015 0.0491 -11.401 0.031 0.009 0.176 0.019 0.016 103.6 26.9 20.1 0.59 0.31 0.20 +FBS0203+374 330722897089067392 sdB 28744 303 5.47 0.04 0.150 1.0701 0.0367 -10.984 0.044 0.004 0.214 0.008 0.007 28.0 2.7 2.6 0.49 0.06 0.06 +FBS0206+428 351633546665907200 sdB 25735 251 5.14 0.03 0.135 0.9280 0.0366 -11.019 0.006 0.007 0.229 0.009 0.009 20.6 2.4 2.2 0.26 0.04 0.03 +FBS0208+390 332606704106366848 sdB 38743 269 6.15 0.04 0.106 0.7313 0.0419 -11.439 0.008 0.011 0.111 0.007 0.006 24.8 3.5 3.0 0.63 0.10 0.09 +FBS0212+334 326009496898928896 sdB 29697 197 5.63 0.04 0.254 1.2116 0.0350 -10.875 0.012 0.006 0.243 0.007 0.007 41.3 3.0 2.9 0.92 0.11 0.10 +FBS0314+372 235323736345986176 sdB 29283 192 5.42 0.03 0.902 0.8740 0.0403 -11.085 0.007 0.029 0.209 0.010 0.009 28.8 3.3 2.9 0.42 0.06 0.05 +FBS0324+379 234861632224343424 sdB 24809 298 5.27 0.03 0.473 1.3008 0.0340 -10.908 0.009 0.007 0.210 0.006 0.006 15.0 1.8 1.7 0.30 0.03 0.03 +FBS0638+428 963881581386403072 sdB 28090 161 5.29 0.02 0.229 1.1992 0.0344 -10.985 0.042 0.010 0.191 0.006 0.006 20.4 1.9 1.9 0.26 0.03 0.03 +FBS0639+391 944892878136403712 sdB 29658 509 5.53 0.08 0.372 0.8262 0.0358 -11.070 0.008 0.007 0.229 0.010 0.010 36.3 4.5 4.0 0.65 0.15 0.12 +FBS0646+386 944390774983674496 sdB 33238 190 5.63 0.03 0.234 0.7018 0.0473 -11.323 0.020 0.012 0.150 0.011 0.010 24.6 3.9 3.4 0.35 0.06 0.05 +FBS1400+389 1495942160078351744 sdOB 18800 1000 4.71 0.10 0.029 1.4515 0.0345 -10.534 0.020 0.045 0.449 0.011 0.011 22.6 5.5 4.7 0.38 0.10 0.08 +FBS1531+381 1375814952762454272 sdB 29230 125 5.58 0.03 0.029 1.9294 0.0345 -10.805 0.013 0.164 0.181 0.004 0.004 21.5 1.7 1.6 0.46 0.04 0.04 +FBS1715+424 1360139937040515072 sdO 58438 514 6.11 0.03 0.010 2.3950 0.0387 -10.911 0.011 0.009 0.114 0.003 0.003 135.4 6.8 6.4 0.61 0.05 0.05 +FBS1745+437 1349088676950060672 sdB 33601 109 5.56 0.02 0.073 1.0659 0.0262 -11.132 0.008 0.006 0.153 0.004 0.004 26.9 2.0 1.9 0.31 0.03 0.03 +FBS2255+404 1930945626165804032 He-sdOB 48127 277 5.92 0.04 0.355 0.4056 0.0444 -11.490 0.049 0.010 0.176 0.022 0.017 149.9 39.4 28.1 0.95 0.27 0.19 +FBS2307+338 1911572540520290048 He-sdO 50664 390 5.85 0.04 0.219 0.4957 0.0502 -11.435 0.006 0.011 0.165 0.018 0.015 160.2 38.3 28.2 0.70 0.18 0.14 +FBS2347+385 2881551562420806784 sdB 23770 350 5.38 0.06 0.269 3.9390 0.0341 -10.434 0.026 0.011 0.207 0.003 0.003 12.3 1.6 1.6 0.37 0.06 0.05 +Feige114 1858674589447492608 sdOB 37689 189 5.56 0.02 0.148 1.2354 0.0317 -10.983 0.023 0.006 0.186 0.005 0.005 62.5 3.8 3.6 0.46 0.04 0.04 +Feige26 2503706418759709184 He-sdO 65608 912 5.46 0.04 0.010 0.5763 0.0471 -11.247 0.007 0.010 0.218 0.019 0.017 793.7 154.1 121.7 0.50 0.11 0.09 +Feige34 781164326766404736 sdO 62400 330 5.95 0.02 0.145 4.4105 0.1039 -10.645 0.069 0.018 0.113 0.003 0.003 174.4 9.3 8.8 0.42 0.04 0.03 +Feige67 3935488605023787392 sdO 61114 318 5.92 0.01 0.105 2.9833 0.0735 -10.739 0.010 0.039 0.136 0.004 0.004 232.9 13.0 12.0 0.56 0.04 0.04 +GALEXJ00468+1956 2801277176253968640 sdB 32891 111 5.84 0.02 0.200 0.9281 0.0413 -11.213 0.041 0.008 0.146 0.007 0.006 22.2 2.5 2.3 0.53 0.06 0.05 +GALEXJ00476+3123 360511037906831872 sdB 31069 166 5.65 0.03 0.207 1.0593 0.0383 -11.149 0.042 0.011 0.148 0.006 0.006 18.4 2.0 1.9 0.36 0.04 0.04 +GALEXJ00498+3522 363795760175504768 sdOB 36551 243 5.74 0.04 0.063 0.8767 0.0412 -11.251 0.010 0.016 0.142 0.007 0.007 32.5 3.7 3.3 0.41 0.06 0.05 +GALEXJ01012+3125 312628749626419328 sdB 28202 155 5.45 0.02 0.063 1.8070 0.0362 -10.788 0.010 0.017 0.201 0.005 0.004 22.9 1.8 1.7 0.41 0.03 0.03 +GALEXJ01194+4901 400211958948711552 He-sdOB 43720 510 5.86 0.21 0.313 1.2614 0.0326 -10.965 0.017 0.012 0.189 0.005 0.005 117.7 8.6 8.0 0.95 0.59 0.37 +GALEXJ01509+3107 304311150320629376 sdB 30183 189 5.84 0.04 0.130 1.3955 0.0367 -11.041 0.004 0.008 0.145 0.004 0.004 15.6 1.7 1.7 0.53 0.06 0.06 +GALEXJ01543+4905 357580873780641920 sdB 32100 410 5.50 0.32 0.452 1.7860 0.0250 -10.871 0.008 0.008 0.166 0.003 0.003 26.4 2.1 2.1 0.32 0.35 0.17 +GALEXJ02069+1438 77515058657678592 sdB 30310 660 5.77 0.06 0.132 2.2104 0.0447 -10.881 0.010 0.028 0.133 0.003 0.003 13.3 1.9 1.9 0.38 0.06 0.05 +GALEXJ02163+2759 107585292928397568 sdB 25480 450 5.35 0.05 0.155 1.5540 0.0313 -10.767 0.028 0.013 0.244 0.005 0.005 22.5 2.4 2.3 0.49 0.07 0.06 +GALEXJ02328+4411 341195058150383104 sdB 33260 420 5.73 0.10 0.237 1.2611 0.0577 -11.082 0.011 0.007 0.145 0.007 0.007 23.1 2.9 2.7 0.41 0.12 0.09 +GALEXJ04158+0154 3259060049366022400 sdBV 34773 123 5.79 0.02 0.359 1.5335 0.0402 -11.003 0.014 0.006 0.144 0.004 0.004 27.1 2.1 2.0 0.46 0.04 0.04 +GALEXJ04205+0120 3255780171819962496 He-sdO 46050 910 5.97 0.16 0.081 2.4658 0.0620 -10.816 0.012 0.006 0.137 0.004 0.004 76.2 7.5 6.9 0.64 0.29 0.20 +GALEXJ04593-0228 3225359193340812288 sdB 30613 608 5.70 0.12 0.062 1.1390 0.0412 -11.197 0.033 0.008 0.124 0.005 0.005 12.0 2.0 1.9 0.28 0.09 0.07 +GALEXJ05369+3955 190970433715259904 He-sdOB 38898 169 5.79 0.04 0.507 1.3436 0.0332 -11.007 0.006 0.008 0.164 0.005 0.004 55.1 3.3 3.1 0.60 0.07 0.06 +GALEXJ05557+6408 287018271958898560 sdO 45600 3380 5.73 0.39 0.462 1.9389 0.0248 -10.932 0.007 0.023 0.134 0.003 0.003 70.1 23.2 18.7 0.35 0.51 0.21 +GALEXJ06134+3420 3452237404778065152 sdOB 34250 390 5.75 0.10 0.432 1.7373 0.0329 -10.935 0.010 0.010 0.148 0.003 0.003 27.1 2.2 2.1 0.45 0.12 0.10 +GALEXJ063952.00+515658.00 992534888766785024 sdB 30400 340 5.58 0.13 0.065 3.0845 0.0455 -10.552 0.031 0.006 0.202 0.004 0.004 31.2 2.2 2.1 0.56 0.20 0.15 +GALEXJ06437+3201 937248901501446272 sdB 26956 303 5.12 0.04 0.331 1.0644 0.0448 -10.873 0.061 0.008 0.276 0.012 0.011 36.0 3.9 3.5 0.37 0.05 0.05 +GALEXJ06463+2920 3386622158606040960 sdOB 41489 229 6.16 0.03 0.073 2.1178 0.0437 -10.998 0.009 0.016 0.105 0.003 0.003 29.3 2.0 1.9 0.58 0.05 0.05 +GALEXJ07013+5329 981727582818800128 He-sdO 67230 3880 5.60 0.22 0.117 0.3925 0.0431 -11.375 0.012 0.005 0.238 0.029 0.023 1038.8 393.0 282.0 0.83 0.61 0.35 +GALEXJ07104+2333 3368383116127317120 sdB 55420 24300 5.21 0.43 0.724 0.5599 0.0242 -11.119 0.071 0.016 0.299 0.013 0.013 756.7 2464.1 679.2 0.53 0.90 0.33 +GALEXJ07108+5624 988436459174352512 sdB 39970 980 5.91 0.14 0.094 0.9733 0.0521 -11.251 0.009 0.005 0.128 0.007 0.007 37.5 6.1 5.2 0.49 0.20 0.14 +GALEXJ07248+1923 3362730178953977472 sdB 25777 334 5.25 0.03 0.172 0.9219 0.0378 -11.069 0.010 0.006 0.205 0.009 0.008 16.7 2.2 2.1 0.27 0.04 0.04 +GALEXJ07380+2624 869050009160765056 sdB 29740 400 5.48 0.06 0.097 0.8730 0.0449 -11.164 0.028 0.008 0.172 0.009 0.009 20.7 3.0 2.6 0.33 0.07 0.06 +GALEXJ07445+3021 879166065892619904 sdB 27910 470 5.42 0.08 0.107 0.8053 0.0407 -11.137 0.006 0.006 0.201 0.011 0.010 22.0 3.2 2.9 0.39 0.09 0.08 +GALEXJ07489+3042 879237740307303040 sdB 30760 830 5.71 0.17 0.143 1.3610 0.0322 -11.036 0.014 0.021 0.150 0.004 0.004 18.0 2.7 2.5 0.42 0.20 0.14 +GALEXJ07581-0432 3068507812327598208 He-sdOB 41360 530 5.85 0.26 0.015 1.7568 0.0429 -10.966 0.006 0.006 0.136 0.004 0.004 48.9 3.8 3.6 0.48 0.39 0.22 +GALEXJ08069+1527 654866823401111168 sdBV 29410 610 5.44 0.12 0.138 0.6909 0.0380 -11.136 0.024 0.013 0.234 0.014 0.012 37.0 5.6 4.9 0.55 0.19 0.14 +GALEXJ080929.46+054843.65 3095093419370170368 sdB 21290 230 4.89 0.05 0.091 0.9665 0.0437 -10.881 0.015 0.026 0.301 0.014 0.013 16.7 2.3 2.1 0.26 0.05 0.04 +GALEXJ08120+0703 3097524714456788992 sdB 35590 620 5.75 0.10 0.010 1.1105 0.0486 -11.113 0.013 0.007 0.154 0.007 0.007 34.1 4.3 3.8 0.49 0.14 0.11 +GALEXJ08125+1601 655674865665718656 sdB 31580 490 5.56 0.13 0.153 1.2438 0.0463 -10.957 0.017 0.029 0.196 0.008 0.007 34.5 3.8 3.5 0.51 0.18 0.14 +GALEXJ08275+1753 662146419308286976 sdB 29550 950 5.55 0.09 0.099 1.1357 0.0438 -11.100 0.014 0.010 0.155 0.006 0.006 16.4 3.0 2.7 0.31 0.08 0.06 +GALEXJ08342+0712 595824702553000448 sdB 29870 560 5.56 0.12 0.052 0.9332 0.0402 -11.148 0.007 0.006 0.169 0.008 0.007 20.4 2.9 2.6 0.38 0.13 0.10 +GALEXJ09568+1422 615674873163301248 He-sdO 49176 242 5.80 0.03 0.072 0.6472 0.0466 -11.226 0.011 0.008 0.204 0.016 0.014 218.5 35.1 28.6 0.96 0.17 0.14 +GALEXJ10415+1842 3986138020473930368 sdB 34890 680 5.80 0.10 0.054 2.0138 0.0531 -10.876 0.009 0.010 0.147 0.004 0.004 28.6 3.1 2.9 0.49 0.13 0.11 +GALEXJ11009+1055 3868418219635118080 sdB 31970 410 5.87 0.10 0.060 1.4054 0.0520 -11.092 0.008 0.008 0.128 0.005 0.005 15.3 2.0 1.9 0.44 0.12 0.10 +GALEXJ11238+2336 3992841536709888640 sdB 27025 338 5.15 0.03 0.035 0.8788 0.0403 -11.014 0.012 0.004 0.244 0.012 0.011 28.4 3.5 3.1 0.31 0.04 0.04 +GALEXJ12521+1151 3927916302803458304 sdB 30842 297 5.45 0.05 0.051 0.6531 0.0492 -11.281 0.010 0.018 0.178 0.015 0.013 25.7 4.7 3.9 0.33 0.07 0.06 +GALEXJ14251+2022 1240306604269576704 sdOB 36873 95 6.04 0.03 0.145 0.8432 0.0415 -11.265 0.026 0.008 0.143 0.008 0.007 33.7 3.9 3.4 0.81 0.11 0.09 +GALEXJ15352+3447 1374058963973357696 sdOB 38575 338 5.70 0.04 0.025 0.6408 0.0354 -11.327 0.010 0.006 0.163 0.010 0.009 52.9 6.8 5.8 0.49 0.08 0.07 +GALEXJ16283+2729 1305126525580012672 sdB 25380 3520 5.31 0.12 0.124 1.1887 0.0295 -10.895 0.009 0.007 0.238 0.006 0.006 21.0 14.4 9.6 0.42 0.14 0.11 +GALEXJ16446-0000 4382904797178453504 sdB 26586 400 5.28 0.04 0.385 1.4584 0.0249 -10.821 0.006 0.007 0.229 0.004 0.004 23.6 2.2 2.1 0.37 0.04 0.04 +GALEXJ17278+1644 4550114402362108416 sdB 28210 550 5.27 0.09 0.676 1.1554 0.0579 -10.759 0.062 0.012 0.327 0.017 0.016 60.7 8.4 7.3 0.73 0.19 0.15 +GALEXJ17365+0736 4487346891305390592 sdB 28100 390 5.43 0.07 0.412 1.3944 0.0273 -10.857 0.010 0.016 0.221 0.005 0.005 27.4 2.4 2.3 0.48 0.09 0.08 +GALEXJ17382+2634 4594148468665436672 sdB 22880 800 5.56 0.10 0.232 1.2811 0.0232 -11.110 0.007 0.017 0.135 0.003 0.003 4.5 1.6 1.5 0.24 0.07 0.05 +GALEXJ19265+4930 2129777323205768448 sdBV 29753 368 5.35 0.06 0.020 0.7855 0.0275 -11.151 0.009 0.007 0.199 0.007 0.007 27.9 2.9 2.7 0.32 0.06 0.05 +GALEXJ20069+1442 1806906627074342016 sdOB 38079 376 6.01 0.06 0.191 1.2864 0.0381 -11.112 0.031 0.010 0.133 0.005 0.004 33.4 2.8 2.7 0.66 0.11 0.09 +GALEXJ20568+0335 1731435633531386752 sdO 40350 1130 5.55 0.09 0.107 0.6749 0.0444 -11.212 0.007 0.041 0.202 0.014 0.013 97.2 18.6 15.3 0.53 0.15 0.12 +GALEXJ21035+3035 1852616039853485824 sdB 35537 105 5.91 0.02 0.168 2.5294 0.0315 -10.841 0.020 0.008 0.126 0.003 0.003 22.8 1.5 1.5 0.47 0.03 0.03 +GALEXJ21226+0558 1738623755222448640 sdB 23340 310 5.13 0.05 0.275 1.0090 0.0266 -10.865 0.017 0.044 0.299 0.008 0.008 23.8 2.3 2.2 0.44 0.06 0.06 +GALEXJ21244-0122 2686048087080526464 sdB 27667 189 5.46 0.02 1.995 1.0288 0.0387 -10.811 0.202 0.081 0.283 0.011 0.010 42.3 3.8 3.5 0.85 0.08 0.07 +GALEXJ21271+0011 2687870218366060416 sdB 30082 106 5.54 0.02 0.902 0.9297 0.0376 -11.017 0.106 0.067 0.195 0.008 0.008 28.0 2.8 2.6 0.48 0.05 0.05 +GD300 828120310859359104 He-sdO 50354 239 5.95 0.03 0.197 1.7381 0.0464 -10.891 0.035 0.017 0.162 0.005 0.005 151.2 9.0 8.3 0.85 0.08 0.07 +GD319 1570548009752602240 sdB 32895 279 5.71 0.04 0.051 4.0394 0.0404 -10.781 0.467 0.008 0.090 0.002 0.002 8.6 1.5 1.4 0.15 0.03 0.03 +HD265435 937565831431448192 sdOB 34033 138 5.50 0.02 0.010 2.2159 0.0554 -10.689 0.031 0.009 0.205 0.006 0.005 50.8 3.1 2.9 0.49 0.04 0.04 +HD345431 1833281127895263872 sdOB 35942 96 5.91 0.02 0.010 3.5455 0.0488 -10.685 0.009 0.007 0.129 0.003 0.003 25.0 1.6 1.6 0.50 0.03 0.03 +HE1415-0309 3645920088861401216 sdB 29520 500 5.56 0.05 0.240 0.4509 0.0743 -11.468 0.024 0.005 0.166 0.032 0.023 18.8 8.3 5.2 0.37 0.17 0.10 +HE1459-0234 6339679321569685504 sdOB 34244 991 5.25 0.15 1.496 0.9140 0.0281 -10.945 0.103 0.025 0.263 0.008 0.008 85.3 11.8 10.6 0.45 0.19 0.13 +HE2201-0001 2680457551489346944 sdB 27062 500 5.51 0.05 0.176 0.5584 0.0780 -11.493 0.008 0.010 0.128 0.021 0.016 7.8 3.1 2.3 0.19 0.08 0.05 +HS0016+0044 2547139876837313920 sdB 28264 500 5.38 0.05 0.575 0.6463 0.0449 -11.069 0.052 0.023 0.279 0.021 0.018 44.7 7.9 6.4 0.68 0.14 0.11 +HS0023+3049 2862194144817359872 sdB 31036 91 5.67 0.02 0.204 0.8539 0.0370 -11.157 0.028 0.013 0.179 0.008 0.008 26.8 2.9 2.6 0.55 0.06 0.06 +HS0025+3423 365939429892433920 sdOB 34935 121 5.85 0.02 0.229 0.8143 0.0675 -11.362 0.012 0.009 0.118 0.011 0.009 18.7 3.8 3.1 0.36 0.07 0.06 +HS0035+3034 2858607022491460096 sdOB 36900 900 5.75 0.10 0.202 0.6507 0.0621 -11.500 0.010 0.007 0.108 0.012 0.010 19.4 5.0 3.9 0.24 0.09 0.06 +HS0233+3037 132944115577925504 sdB 29213 148 5.67 0.03 0.479 1.6361 0.0355 -10.902 0.005 0.008 0.170 0.004 0.004 18.9 1.7 1.7 0.49 0.05 0.04 +HS0258+3003 123108816565129344 sdO 55880 4670 6.25 0.18 0.531 1.1549 0.0425 -11.325 0.005 0.011 0.091 0.004 0.004 73.1 28.2 21.8 0.54 0.28 0.19 +HS0352+1019 3302955130527310464 sdB 25291 278 5.11 0.04 0.543 1.3481 0.0285 -10.891 0.014 0.006 0.211 0.005 0.005 16.4 1.7 1.7 0.21 0.03 0.03 +HS0357+0133 3259569020169965312 sdB 31164 210 5.82 0.05 0.902 1.2222 0.0280 -11.013 0.018 0.011 0.176 0.005 0.004 26.4 2.0 2.0 0.75 0.10 0.09 +HS0600+6602 1008782681328282112 sdOB 36846 432 5.97 0.09 0.398 0.5768 0.0551 -11.501 0.054 0.011 0.121 0.013 0.011 24.4 5.7 4.4 0.50 0.17 0.12 +HS0741+3818 919963474904219776 sdB 30190 228 5.37 0.03 0.184 0.6170 0.0373 -11.156 0.011 0.007 0.251 0.016 0.014 46.8 6.5 5.5 0.54 0.08 0.07 +HS1710+1614 4546882216133354752 sdB 34826 500 5.72 0.05 0.209 0.5274 0.0486 -11.510 0.016 0.007 0.130 0.013 0.011 22.2 5.1 4.0 0.32 0.08 0.07 +HS1831+6432 2256432438426909952 sdOB 36000 900 5.85 0.10 0.140 0.8609 0.0316 -11.355 0.013 0.004 0.113 0.005 0.004 19.4 2.9 2.7 0.33 0.09 0.07 +HS1837+5913 2154810316748450432 He-sdOB 40232 154 5.61 0.04 0.067 0.7917 0.0319 -11.243 0.005 0.010 0.160 0.007 0.006 60.5 5.4 4.8 0.38 0.05 0.05 +HS2029+0301 4232792524791811968 sdB 31100 1000 5.60 0.20 0.138 0.9269 0.0579 -11.295 0.051 0.007 0.121 0.008 0.007 12.3 2.8 2.5 0.22 0.13 0.08 +HS2100+1710 1764138098639251456 sdOB 34100 900 6.05 0.10 0.243 0.7036 0.0368 -11.312 0.009 0.024 0.154 0.009 0.008 28.7 4.8 4.2 0.97 0.28 0.21 +HS2158+2137 1782619686510352128 sdB 35592 487 6.10 0.09 0.251 1.6035 0.0374 -11.036 0.007 0.010 0.127 0.004 0.004 23.3 2.2 2.2 0.74 0.18 0.14 +HS2213+1336 2734200064947455232 sdB 24682 405 5.14 0.04 0.305 0.3554 0.0447 -11.227 0.005 0.009 0.370 0.053 0.042 45.6 14.6 10.1 0.69 0.23 0.16 +HS2225+2220 1875278658119889408 sdB 31500 800 5.85 0.10 0.243 0.6413 0.0587 -11.576 0.007 0.009 0.092 0.009 0.008 7.5 2.3 2.0 0.22 0.08 0.06 +HS2231+2441 1877320760449993216 sdB 30173 115 5.66 0.02 0.094 1.1041 0.0453 -11.025 0.018 0.008 0.189 0.008 0.008 26.7 2.7 2.5 0.60 0.06 0.06 +HS2240+0136 2654793575707334784 sdB 31766 111 6.06 0.02 0.221 1.5280 0.0366 -11.085 0.010 0.015 0.119 0.004 0.003 13.0 1.6 1.5 0.59 0.05 0.04 +HS2242+3206 1890677009230168704 sdB 31010 47 5.71 0.01 0.248 1.4531 0.0292 -10.977 0.005 0.009 0.161 0.004 0.004 21.6 1.7 1.6 0.49 0.03 0.03 +HS2357+2201 2847977322031768832 sdB 27629 500 5.55 0.05 0.124 1.2038 0.0359 -11.021 0.010 0.010 0.176 0.006 0.005 16.2 2.1 2.0 0.40 0.06 0.05 +HZ11 3287144634355536768 sdO 42882 236 6.01 0.03 0.525 1.0245 0.0421 -11.269 0.038 0.010 0.116 0.005 0.005 40.8 3.9 3.5 0.50 0.06 0.05 +HZ3 3303143628052101120 He-sdOB 43077 231 5.57 0.05 0.376 2.2644 0.0557 -10.851 0.004 0.023 0.139 0.004 0.004 59.4 3.6 3.4 0.26 0.04 0.04 +HZ44 1473687671071803520 sdOB 38012 192 5.46 0.03 0.123 2.7350 0.0543 -10.634 0.021 0.025 0.193 0.004 0.004 69.5 3.5 3.3 0.39 0.04 0.04 +KBS13 2051770507972278016 sdB 31075 111 5.77 0.02 0.295 1.7302 0.0237 -10.885 0.048 0.007 0.165 0.003 0.003 22.8 1.6 1.6 0.58 0.04 0.04 +KIC10149211 2128554563197280512 sdB 30627 248 5.59 0.05 0.617 0.6541 0.0337 -11.168 0.065 0.016 0.224 0.012 0.011 39.5 4.8 4.2 0.71 0.12 0.10 +KIC10553698 2086441927825846656 sdB 29231 320 5.26 0.05 0.302 0.7829 0.0269 -11.151 0.044 0.002 0.199 0.007 0.007 26.0 2.6 2.5 0.26 0.04 0.04 +KIC10670103 2128836553569442816 sdBV 25361 632 5.59 0.07 0.207 0.4026 0.0402 -11.339 0.042 0.005 0.252 0.028 0.023 23.6 6.3 4.8 0.90 0.27 0.20 +KIC12021724 2135353702585217920 sdB 28180 292 5.42 0.04 0.178 0.6326 0.0288 -11.253 0.015 0.005 0.195 0.010 0.009 21.6 2.7 2.5 0.37 0.06 0.05 +KIC2697388 2099149567821051904 sdBV 24320 90 5.42 0.02 0.211 0.7881 0.0270 -11.144 0.009 0.010 0.202 0.007 0.007 12.8 1.7 1.6 0.39 0.04 0.04 +KIC3527751 2100027626635533056 sdBV 27831 336 5.08 0.04 0.260 0.8216 0.0306 -11.082 0.015 0.006 0.223 0.009 0.008 26.8 2.9 2.6 0.22 0.04 0.03 +KIC7353409 2102745688098547840 sdOB 43143 702 5.35 0.05 0.106 0.6843 0.0306 -11.203 0.017 0.008 0.203 0.010 0.009 127.7 15.1 13.2 0.34 0.06 0.05 +KIC8054179 2079009641541181312 He-sdOB 40933 152 5.94 0.03 0.367 1.4789 0.0224 -11.128 0.044 0.011 0.112 0.003 0.003 31.5 1.8 1.7 0.40 0.04 0.04 +KIC9543660 2079522048319286528 sdOB 38592 137 5.85 0.02 0.157 1.2421 0.0239 -11.001 0.035 0.013 0.176 0.004 0.004 61.7 3.0 2.8 0.80 0.05 0.05 +KPD0005+5106 395429431270137728 sdO 200000 20000 6.70 0.30 0.123 2.4234 0.0355 -11.093 0.012 0.007 0.074 0.002 0.002 7789.3 3609.3 2662.3 0.99 0.98 0.49 +KPD0033+5229 416348224099839104 sdO 40718 123 5.86 0.02 0.417 0.6669 0.0483 -11.445 0.041 0.009 0.119 0.009 0.008 34.7 5.8 4.7 0.37 0.07 0.06 +KPD0106+5227 404959035980962944 sdB 32501 335 5.24 0.05 1.000 0.5578 0.0330 -11.160 0.036 0.009 0.275 0.017 0.015 75.6 10.5 8.8 0.48 0.09 0.08 +KPD0111+5200 404172060534423296 sdO 59320 1870 6.05 0.06 0.741 0.7241 0.0560 -11.547 0.014 0.008 0.087 0.008 0.007 83.4 18.6 14.9 0.31 0.07 0.06 +KPD0549+1948 3398928751737464192 sdO 74993 3700 6.50 0.02 0.452 1.2968 0.0380 -11.337 0.011 0.012 0.079 0.003 0.003 175.2 38.9 33.1 0.71 0.06 0.06 +KPD0550+1922 3398852881140229632 sdB 29947 229 5.68 0.04 0.385 1.0963 0.0312 -11.034 0.010 0.015 0.188 0.006 0.005 25.4 2.2 2.1 0.62 0.07 0.07 +KPD0552+1903 3398598348493762944 He-sdO 67116 829 5.40 0.05 1.288 0.5562 0.0267 -11.103 0.013 0.012 0.313 0.016 0.014 1785.7 205.0 179.8 0.90 0.15 0.13 +KPD0640+1412 3355897092143865088 sdB 36432 180 5.68 0.04 0.902 1.1127 0.0308 -11.094 0.009 0.013 0.161 0.005 0.005 40.8 2.9 2.7 0.45 0.06 0.05 +KPD0716+0258 3139042514040855296 sdB 28812 327 5.49 0.05 0.240 0.6932 0.0318 -11.092 0.008 0.007 0.258 0.013 0.011 41.3 4.8 4.2 0.75 0.12 0.10 +KPD2051+3544 1869904107861540864 sdB 31665 200 5.96 0.05 0.359 0.8027 0.0331 -11.312 0.036 0.008 0.135 0.006 0.006 16.4 2.0 1.9 0.60 0.09 0.08 +KUV02129+2907 108002248353357312 sdB 24230 191 5.58 0.02 0.279 1.9203 0.0425 -10.875 0.008 0.003 0.153 0.004 0.004 7.3 1.5 1.5 0.33 0.03 0.03 +KUV02281+2730 127674641678296704 sdO 47501 290 5.90 0.02 0.351 1.0255 0.0415 -11.334 0.007 0.008 0.100 0.005 0.004 46.0 4.3 3.9 0.29 0.04 0.03 +KUV02290+3321 134510477267997952 sdB 24828 285 5.62 0.04 0.320 0.8619 0.0537 -11.142 0.028 0.009 0.184 0.012 0.011 11.5 2.2 2.0 0.51 0.09 0.08 +KUV02445+3633 141428363911552384 He-sdOB 44029 175 5.83 0.03 0.153 1.4784 0.0551 -10.931 0.004 0.005 0.176 0.007 0.007 104.8 8.6 7.7 0.77 0.09 0.08 +KUV02587-0252 5186434732342771968 sdB 25821 386 5.11 0.03 0.232 1.2470 0.0308 -10.897 0.009 0.007 0.225 0.006 0.006 20.2 2.1 2.1 0.24 0.03 0.03 +KUV04233+1502 3311181332928254464 sdO 68925 1135 5.32 0.05 1.531 0.7665 0.0221 -11.004 0.010 0.013 0.287 0.009 0.008 1671.5 151.7 140.2 0.63 0.09 0.08 +KUV04421+1416 3308791681845675136 sdBV 34862 242 5.94 0.04 1.603 1.4853 0.0289 -10.950 0.027 0.013 0.166 0.004 0.004 36.6 2.3 2.2 0.88 0.09 0.09 +KUV04456+1502 3308929464395407104 He-sdOB 45687 332 5.67 0.04 1.148 0.7881 0.0409 -11.261 0.043 0.024 0.154 0.009 0.008 93.1 10.8 9.4 0.41 0.06 0.06 +KUV04498+1727 3406444218653682560 sdB 24815 411 5.20 0.05 1.216 0.5732 0.0564 -11.121 0.028 0.009 0.292 0.032 0.026 29.1 7.1 5.4 0.49 0.13 0.10 +KUV05072+1249 3388371103647349632 sdB 32372 171 5.96 0.04 1.259 1.1843 0.0523 -11.225 0.005 0.015 0.112 0.005 0.005 12.3 1.8 1.8 0.41 0.06 0.05 +KUV06239+2811 3432828791165658880 sdB 23723 573 5.07 0.06 0.955 0.4704 0.0461 -11.007 0.010 0.004 0.460 0.050 0.041 60.3 15.4 11.5 0.91 0.26 0.19 +KUV06290+2813 3434099173772378112 He-sdO 45865 247 5.57 0.04 0.422 0.6738 0.0456 -11.304 0.026 0.008 0.163 0.012 0.011 106.0 16.1 13.2 0.36 0.07 0.06 +KUV07592+3931 921064055980216320 sdOB 35719 172 5.59 0.03 0.051 0.5042 0.0478 -11.331 0.004 0.006 0.205 0.022 0.018 61.5 13.7 10.3 0.60 0.14 0.11 +KUV07596+4123 921531554580422016 sdO 45319 2000 5.77 0.20 0.288 0.5864 0.0499 -11.363 0.038 0.005 0.163 0.015 0.013 101.3 28.1 21.9 0.58 0.37 0.22 +KUV16160+4120 1380875729907633408 He-sdOB 40565 1112 6.01 0.26 0.146 0.2747 0.0526 -11.748 0.019 0.009 0.144 0.034 0.023 50.5 27.5 15.6 0.79 0.85 0.40 +KUV16256+4034 1332896306646572160 sdBV 23560 410 5.44 0.07 0.039 2.3654 0.0340 -10.632 0.017 0.012 0.215 0.004 0.004 12.8 1.7 1.7 0.46 0.09 0.07 +KUV18312+6431 2256432335347693696 sdB 29866 1000 5.54 0.16 0.138 0.3205 0.0462 -11.576 0.006 0.007 0.184 0.031 0.023 24.2 9.7 6.4 0.43 0.27 0.16 +Kepler-451 2080063931448749824 sdBV 29600 500 5.43 0.05 0.117 2.4758 0.0316 -10.613 0.017 0.015 0.219 0.003 0.003 33.0 2.8 2.7 0.47 0.06 0.06 +LAMOSTJ000824.52+490501.9 393589879591384576 sdB 29448 307 5.45 0.05 0.359 0.6389 0.0432 -11.298 0.041 0.007 0.175 0.013 0.011 20.6 3.5 3.0 0.31 0.07 0.05 +LAMOSTJ001144.75+464806.7 392942881419391872 He-sdOB 45717 206 5.56 0.03 0.309 0.7103 0.0396 -11.192 0.004 0.006 0.201 0.012 0.011 157.9 19.5 16.4 0.53 0.08 0.07 +LAMOSTJ001306.41+491148.9 393652139438978304 He-sdOB 43628 206 6.32 0.04 0.211 0.5515 0.0713 -11.634 0.043 0.013 0.093 0.014 0.011 28.0 9.0 6.2 0.66 0.22 0.15 +LAMOSTJ001631.08+315740.5 2863196315306344832 sdB 28118 325 5.22 0.04 1.175 0.6659 0.0404 -11.036 0.041 0.017 0.297 0.019 0.017 49.4 7.2 6.0 0.53 0.09 0.08 +LAMOSTJ001651.95+520847.4 395157267782903808 sdB 31383 234 5.70 0.06 0.407 0.4047 0.0552 -11.484 0.040 0.004 0.179 0.028 0.021 28.0 9.7 6.5 0.59 0.23 0.15 +LAMOSTJ001655.34+511349.7 394991241522199040 sdB 33816 268 5.63 0.05 0.513 0.4742 0.0465 -11.431 0.038 0.009 0.172 0.019 0.016 34.9 8.2 6.2 0.46 0.12 0.09 +LAMOSTJ001917.36+403008.2 380384779299991424 sdB 29105 410 5.33 0.07 0.403 0.3941 0.0523 -11.350 0.072 0.014 0.248 0.038 0.029 39.7 13.4 9.0 0.48 0.19 0.13 +LAMOSTJ001954.03+510505.6 394948356271554816 He-sdO 73002 5928 6.01 0.15 0.335 0.6566 0.0665 -11.672 0.006 0.013 0.072 0.008 0.007 134.0 61.2 43.3 0.20 0.10 0.07 +LAMOSTJ002124.79+402857.1 380338531092183424 sdB 28064 375 5.46 0.06 0.178 0.4903 0.0403 -11.237 0.044 0.008 0.262 0.024 0.020 38.1 7.6 6.0 0.72 0.18 0.14 +LAMOSTJ002327.19+510749.9 394843322846749824 sdB 26874 524 5.35 0.05 0.313 0.5821 0.0420 -11.282 0.047 0.012 0.199 0.015 0.014 18.5 3.7 3.1 0.32 0.07 0.06 +LAMOSTJ002408.46+560139.2 421328839978415616 sdOB 36247 198 5.98 0.03 0.813 0.7370 0.0406 -11.361 0.009 0.018 0.132 0.008 0.007 26.8 3.6 3.1 0.60 0.09 0.08 +LAMOSTJ002545.50+313529.4 2862287843823854848 sdB 27087 322 5.39 0.03 0.232 0.5118 0.0447 -11.221 0.013 0.005 0.260 0.025 0.021 32.7 6.9 5.4 0.61 0.13 0.10 +LAMOSTJ002606.79+443318.2 382781542850500352 sdOB 37229 281 5.97 0.05 0.056 0.3836 0.0680 -11.738 0.010 0.011 0.104 0.022 0.016 18.5 8.9 5.4 0.37 0.18 0.11 +LAMOSTJ002919.04+525831.6 416403783797286784 sdOB 42205 773 5.82 0.07 0.525 0.3227 0.0616 -11.556 0.167 0.007 0.190 0.045 0.030 102.8 54.7 30.8 0.87 0.49 0.28 +LAMOSTJ003801.72+343156.2 365002268028633600 He-sdOB 42088 205 5.43 0.04 0.403 1.1197 0.0304 -11.046 0.005 0.010 0.179 0.005 0.005 90.0 5.5 5.2 0.31 0.04 0.04 +LAMOSTJ003805.43+434450.4 387661209812972928 sdOB 37953 275 6.13 0.05 0.182 0.6732 0.0585 -11.496 0.016 0.008 0.105 0.010 0.009 20.6 4.4 3.5 0.54 0.13 0.10 +LAMOSTJ004139.06+420713.5 381370731998505472 sdOB 37040 331 5.93 0.06 0.164 0.3926 0.0656 -11.574 0.013 0.005 0.150 0.030 0.022 38.1 16.8 10.3 0.70 0.33 0.20 +LAMOSTJ004906.06+395021.0 368884712306195584 sdB 31726 224 6.03 0.05 0.150 0.7345 0.0401 -11.276 0.043 0.008 0.160 0.009 0.008 23.2 3.2 2.8 1.00 0.17 0.15 +LAMOSTJ005821.83+553750.9 423505288886486272 sdB 21132 133 5.03 0.02 0.550 1.1284 0.0220 -10.633 0.014 0.009 0.455 0.009 0.009 37.1 2.3 2.2 0.81 0.06 0.05 +LAMOSTJ010345.21+471024.3 401237459701979776 sdOB 38611 375 5.89 0.06 0.372 0.5279 0.0598 -11.556 0.036 0.012 0.117 0.015 0.012 27.3 7.6 5.5 0.39 0.12 0.09 +LAMOSTJ010940.46+524908.6 404958378847936000 sdOB 36268 220 6.18 0.05 1.175 0.5732 0.0880 -11.545 0.005 0.019 0.110 0.020 0.015 18.9 7.6 4.9 0.68 0.28 0.18 +LAMOSTJ011404.27+335652.2 314106974290607104 sdB 31720 444 5.19 0.07 1.189 0.6121 0.0305 -11.023 0.054 0.011 0.338 0.018 0.016 103.8 12.7 11.1 0.65 0.14 0.11 +LAMOSTJ012609.24+454716.6 397395014455786624 sdB 29245 622 5.29 0.12 0.279 0.8432 0.0390 -11.192 0.026 0.012 0.169 0.008 0.008 18.9 2.9 2.6 0.20 0.07 0.06 +LAMOSTJ013134.51+323723.7 316170482737881728 sdO 62176 1092 5.93 0.05 0.039 0.6771 0.0565 -11.436 0.006 0.007 0.120 0.011 0.009 193.7 39.8 31.3 0.45 0.11 0.08 +LAMOSTJ014408.84+540210.7 408127652396870400 sdO 50787 556 5.54 0.03 1.230 0.4503 0.0495 -11.393 0.076 0.017 0.192 0.024 0.019 221.2 59.1 42.4 0.47 0.13 0.10 +LAMOSTJ014640.50+411825.8 347453684494319104 He-sdB 28103 130 5.36 0.02 0.182 0.3466 0.0479 -11.311 0.005 0.008 0.313 0.049 0.038 54.7 18.7 12.5 0.82 0.28 0.19 +LAMOSTJ014714.16+023745.3 2512318137425806720 sdOB 35905 273 5.60 0.05 0.923 0.5594 0.0404 -11.210 0.064 0.013 0.239 0.019 0.016 85.2 14.1 11.4 0.83 0.17 0.14 +LAMOSTJ015548.96+413256.1 345949758745792000 sdOB 37940 259 5.74 0.03 0.148 0.6911 0.0466 -11.434 0.019 0.006 0.118 0.009 0.008 25.8 4.2 3.5 0.28 0.05 0.04 +LAMOSTJ015640.41+443443.6 349755232912531072 sdOB 38369 451 5.66 0.07 0.412 0.4093 0.0816 -11.635 0.062 0.010 0.125 0.031 0.021 30.2 16.8 9.3 0.26 0.16 0.09 +LAMOSTJ015835.30+550504.8 504485110543295616 sdO 42578 266 5.99 0.02 1.122 0.7418 0.0334 -11.262 0.012 0.019 0.164 0.008 0.007 79.6 8.0 7.1 0.96 0.10 0.09 +LAMOSTJ020201.84+564342.2 505063728541561344 sdB 31098 205 5.77 0.05 0.700 0.9800 0.0313 -11.118 0.014 0.009 0.172 0.006 0.006 24.9 2.3 2.2 0.64 0.09 0.08 +LAMOSTJ020420.23+292734.8 300019923940638336 sdOB 30083 149 5.95 0.04 0.197 0.6720 0.0662 -11.407 0.035 0.008 0.129 0.014 0.012 12.3 3.2 2.5 0.54 0.14 0.10 +LAMOSTJ020630.69+543108.5 456417279675979008 sdOB 35344 126 5.23 0.02 0.902 0.6475 0.0257 -10.965 0.009 0.011 0.371 0.015 0.014 192.5 16.5 14.7 0.85 0.09 0.08 +LAMOSTJ021534.78+492537.7 355574058902192768 sdOB 38672 262 6.06 0.04 0.733 0.4596 0.0715 -11.541 0.037 0.013 0.137 0.025 0.018 38.0 15.3 9.6 0.79 0.33 0.21 +LAMOSTJ021708.68+434053.0 351536441749571200 sdOB 36880 141 5.92 0.03 0.299 0.6761 0.0528 -11.358 0.006 0.026 0.144 0.012 0.011 34.5 6.2 5.0 0.63 0.12 0.10 +LAMOSTJ021749.89+415835.1 339286202884520064 sdB 31770 168 5.64 0.03 0.279 0.3354 0.0646 -11.433 0.024 0.006 0.244 0.057 0.039 54.5 28.6 16.3 0.95 0.51 0.29 +LAMOSTJ022141.57+540653.4 455558286215251840 sdB 28582 394 5.70 0.06 0.646 0.4280 0.0588 -11.397 0.025 0.008 0.207 0.033 0.025 25.7 9.0 6.1 0.79 0.30 0.20 +LAMOSTJ022512.43+234822.2 101826669497182720 sdO 50765 384 5.64 0.03 0.359 1.3925 0.0406 -11.102 0.008 0.047 0.127 0.004 0.004 96.3 6.7 6.2 0.26 0.03 0.03 +LAMOSTJ022619.89+180729.6 85707760314515712 sdOB 37916 559 5.87 0.10 0.902 1.5037 0.0395 -11.069 0.008 0.014 0.126 0.004 0.004 29.4 2.8 2.6 0.43 0.12 0.09 +LAMOSTJ023316.25+082248.1 20063858119453824 sdB 31466 203 5.79 0.04 0.638 0.8447 0.0489 -11.162 0.011 0.018 0.174 0.011 0.010 26.6 3.7 3.2 0.68 0.11 0.10 +LAMOSTJ023851.64+432309.5 340246759434370048 He-sdO 59021 1501 6.17 0.13 0.080 0.4515 0.0842 -11.790 0.012 0.010 0.079 0.018 0.012 68.7 35.9 20.5 0.34 0.22 0.13 +LAMOSTJ025020.85+491234.0 438686001110484352 sdB 31876 166 5.74 0.04 0.822 0.8226 0.0365 -11.225 0.006 0.011 0.161 0.008 0.007 24.0 2.7 2.5 0.52 0.07 0.07 +LAMOSTJ030236.01+281616.9 116691791828603136 sdOB 39230 192 5.95 0.03 0.569 0.7094 0.0550 -11.464 0.011 0.011 0.108 0.009 0.008 24.6 4.5 3.7 0.38 0.08 0.06 +LAMOSTJ031038.31+470117.5 434997246974962688 sdB 34823 620 5.76 0.13 1.035 0.4384 0.0842 -11.506 0.005 0.020 0.158 0.038 0.025 33.0 17.8 10.0 0.53 0.36 0.20 +LAMOSTJ031151.16+082434.6 13746369248366848 sdB 34920 164 6.06 0.03 1.216 1.6207 0.0250 -10.975 0.013 0.014 0.145 0.003 0.003 28.1 1.7 1.7 0.88 0.07 0.07 +LAMOSTJ031311.81+282735.8 121811255405332352 sdOB 40488 652 5.82 0.07 0.804 1.0647 0.0318 -11.194 0.009 0.009 0.133 0.005 0.004 42.8 4.2 3.8 0.43 0.08 0.07 +LAMOSTJ031318.14+464902.5 435028583061655040 sdOB 35097 458 5.72 0.09 1.175 0.5652 0.0729 -11.433 0.033 0.020 0.139 0.021 0.016 26.4 8.6 6.0 0.37 0.15 0.10 +LAMOSTJ031319.32+284159.8 121824174666929024 sdB 32213 302 5.88 0.08 0.741 0.6906 0.0613 -11.264 0.014 0.011 0.175 0.017 0.014 29.6 6.3 4.9 0.85 0.25 0.19 +LAMOSTJ031541.48+465211.0 434851149371030272 sdOB 40059 404 5.42 0.04 0.776 0.4540 0.0430 -11.328 0.014 0.011 0.229 0.024 0.020 121.7 27.4 20.4 0.51 0.13 0.10 +LAMOSTJ031756.92+322950.4 125093503772825856 sdOB 36093 197 6.11 0.04 0.871 0.9185 0.0454 -11.254 0.029 0.021 0.135 0.007 0.007 27.6 3.3 3.0 0.85 0.12 0.11 +LAMOSTJ032121.97+370009.5 234507383322003072 sdOB 38846 429 6.02 0.06 0.692 0.5166 0.0754 -11.520 0.023 0.018 0.130 0.022 0.017 34.4 12.9 8.4 0.65 0.26 0.17 +LAMOSTJ032133.19+081131.6 11015044926034816 sdB 33853 141 5.88 0.03 0.624 0.7520 0.0489 -11.337 0.038 0.011 0.136 0.010 0.008 21.7 3.4 2.9 0.51 0.09 0.07 +LAMOSTJ032357.44+421614.8 240978868246214400 sdOB 36866 298 5.95 0.05 0.603 0.7593 0.0406 -11.324 0.026 0.010 0.138 0.008 0.007 31.7 4.1 3.6 0.62 0.11 0.09 +LAMOSTJ033309.34+341230.8 221005208733887488 sdOB 34893 173 5.91 0.04 1.349 1.0625 0.0418 -11.181 0.024 0.011 0.138 0.006 0.006 25.2 2.6 2.4 0.56 0.08 0.07 +LAMOSTJ033357.86+265553.8 69784942159807232 sdOB 40066 388 6.08 0.06 0.668 0.6177 0.0757 -11.514 0.007 0.011 0.110 0.015 0.012 28.0 8.5 6.0 0.53 0.18 0.13 +LAMOSTJ033611.40+441925.4 238611138677074560 sdB 27968 814 5.41 0.09 1.000 0.7172 0.0684 -11.334 0.005 0.034 0.144 0.015 0.013 11.3 3.3 2.6 0.19 0.07 0.05 +LAMOSTJ033628.30+460816.5 247823740446444416 sdOB 37852 267 5.95 0.04 1.413 0.7841 0.0545 -11.285 0.030 0.018 0.146 0.011 0.010 39.6 6.3 5.3 0.70 0.13 0.11 +LAMOSTJ033821.59+414404.5 237331822538478592 sdB 27936 263 5.64 0.03 0.638 1.0252 0.0370 -11.095 0.011 0.005 0.174 0.007 0.006 16.5 2.0 1.9 0.48 0.05 0.05 +LAMOSTJ033843.01+302319.5 120354952254440960 sdB 33575 152 5.62 0.04 1.288 0.7281 0.0645 -11.343 0.021 0.011 0.138 0.014 0.011 21.7 4.7 3.7 0.29 0.07 0.06 +LAMOSTJ033847.06+413424.2 237133566847520000 sdB 24806 123 6.06 0.02 0.531 1.6778 0.0318 -11.052 0.006 0.012 0.117 0.003 0.003 4.7 1.4 1.4 0.58 0.04 0.04 +LAMOSTJ033946.63+353246.1 221375331836119552 sdO 64062 1122 5.70 0.04 1.365 0.9556 0.0395 -11.296 0.014 0.011 0.117 0.005 0.005 207.5 23.8 21.2 0.25 0.04 0.04 +LAMOSTJ034029.29+242956.9 68334308365794304 sdB 26583 362 5.78 0.05 0.871 0.6431 0.0624 -11.281 0.049 0.015 0.181 0.019 0.016 14.7 3.7 2.9 0.72 0.19 0.14 +LAMOSTJ034208.81+090220.7 11963171843658240 sdOB 41361 995 5.11 0.08 0.861 0.4186 0.0471 -11.345 0.008 0.017 0.239 0.030 0.024 150.2 43.3 31.4 0.27 0.10 0.07 +LAMOSTJ034237.14+200121.0 63139734399542528 He-sdO 48957 222 5.96 0.05 0.891 0.5633 0.0555 -11.440 0.015 0.014 0.143 0.016 0.013 105.0 24.1 18.0 0.68 0.18 0.14 +LAMOSTJ034405.32+220422.7 64368713521485568 sdB 27591 290 5.27 0.03 0.933 1.1607 0.0351 -10.879 0.024 0.012 0.245 0.008 0.007 31.4 2.8 2.6 0.41 0.05 0.04 +LAMOSTJ035001.86+324433.0 217062978512976000 sdB 32850 202 5.99 0.05 0.804 0.6328 0.1028 -11.476 0.029 0.008 0.117 0.023 0.016 14.3 6.2 4.0 0.49 0.22 0.14 +LAMOSTJ035144.09+365216.7 220091342774317056 sdB 26870 436 5.53 0.05 1.905 1.0776 0.0453 -11.067 0.028 0.017 0.170 0.008 0.007 13.6 2.1 1.9 0.36 0.06 0.05 +LAMOSTJ035706.34+362829.4 220172981513287936 sdO 74259 2623 5.92 0.04 0.804 0.8321 0.0388 -11.386 0.019 0.018 0.109 0.006 0.005 326.6 59.5 50.8 0.36 0.06 0.05 +LAMOSTJ040012.58+363545.8 219511728348315520 sdB 24768 438 5.44 0.05 1.259 1.4687 0.0261 -10.856 0.010 0.006 0.209 0.004 0.004 14.8 1.9 1.8 0.44 0.06 0.05 +LAMOSTJ040047.29+171842.0 46608061680943872 sdB 29995 221 5.62 0.04 1.122 0.8219 0.0400 -11.064 0.010 0.013 0.235 0.012 0.011 40.1 4.5 4.0 0.84 0.12 0.11 +LAMOSTJ040242.09+312349.5 169258102725227008 sdOB 37295 313 5.80 0.05 0.933 0.9656 0.0578 -11.301 0.024 0.004 0.114 0.008 0.007 22.8 3.4 2.9 0.30 0.06 0.05 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161 5.83 0.02 1.035 1.3073 0.0377 -11.128 0.069 0.007 0.126 0.004 0.004 28.3 2.3 2.1 0.39 0.04 0.04 +LAMOSTJ042409.66+083317.2 3299455110137611776 sdB 25344 253 5.04 0.02 0.668 1.8993 0.0324 -10.550 0.013 0.019 0.328 0.006 0.006 40.0 2.6 2.5 0.43 0.03 0.03 +LAMOSTJ042700.08-025301.6 3205579387177651072 sdB 25306 753 5.71 0.10 0.058 0.5699 0.0714 -11.447 0.016 0.008 0.139 0.020 0.015 7.1 2.8 2.2 0.36 0.15 0.10 +LAMOSTJ044314.47+231303.4 146588028382865280 sdOB 38051 414 5.61 0.06 1.216 0.5674 0.0424 -11.255 0.025 0.008 0.215 0.017 0.015 86.7 15.1 12.1 0.69 0.16 0.13 +LAMOSTJ044708.74+215327.4 3412738686500055296 sdB 30430 300 5.39 0.08 1.349 0.5693 0.1082 -11.512 0.048 0.013 0.119 0.028 0.019 11.0 5.9 3.5 0.13 0.08 0.05 +LAMOSTJ044748.76+560531.9 274505760917939200 sdOB 35760 371 5.70 0.06 1.567 0.6300 0.0551 -11.285 0.025 0.019 0.183 0.018 0.015 49.2 10.2 7.9 0.61 0.16 0.12 +LAMOSTJ044847.21-040016.9 3200857538788110080 sdB 29884 231 5.57 0.03 0.015 2.0071 0.0412 -10.873 0.010 0.006 0.147 0.004 0.004 15.5 1.6 1.6 0.29 0.03 0.03 +LAMOSTJ045027.67+155909.9 3405118997904684032 He-sdOB 38178 191 5.80 0.04 1.479 0.5651 0.0628 -11.349 0.027 0.022 0.167 0.021 0.017 53.2 14.2 10.2 0.64 0.18 0.13 +LAMOSTJ045557.69+461907.9 254631847728048384 sdB 30041 243 5.78 0.05 1.135 0.9303 0.0358 -11.102 0.023 0.008 0.188 0.008 0.007 25.8 2.7 2.5 0.78 0.12 0.10 +LAMOSTJ045715.16+430320.3 205078336132788352 sdB 27680 540 5.48 0.08 0.871 0.6052 0.0479 -11.218 0.020 0.008 0.221 0.019 0.016 25.8 5.3 4.3 0.54 0.15 0.12 +LAMOSTJ045905.45+393754.2 199210757970191744 sdB 34015 124 5.41 0.03 1.380 0.5258 0.0428 -11.177 0.020 0.011 0.278 0.025 0.021 93.0 17.4 13.5 0.73 0.15 0.12 +LAMOSTJ050238.49+454314.2 206657161813612288 sdB 35157 219 6.06 0.05 1.012 1.0080 0.0426 -11.201 0.026 0.007 0.138 0.006 0.006 26.0 2.8 2.6 0.80 0.12 0.11 +LAMOSTJ050252.26+162647.9 3393408962846662656 sdOB 43997 650 5.37 0.05 0.966 0.5869 0.0426 -11.288 0.015 0.013 0.195 0.015 0.013 127.8 22.1 18.1 0.33 0.07 0.06 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37153 287 5.90 0.05 0.646 0.9989 0.0389 -11.209 0.013 0.013 0.137 0.006 0.005 32.3 3.2 2.9 0.55 0.08 0.07 +LAMOSTJ052258.74+350112.8 183572846467281152 sdB 33283 675 5.48 0.12 1.059 0.8341 0.0541 -11.260 0.034 0.011 0.146 0.010 0.009 23.5 4.2 3.6 0.24 0.09 0.07 +LAMOSTJ052351.37+140443.5 3390235531771243904 sdB 22589 174 5.06 0.02 1.148 0.6548 0.0400 -11.052 0.030 0.012 0.298 0.019 0.017 20.7 3.2 2.8 0.37 0.06 0.05 +LAMOSTJ052354.42-000346.7 3221394624991995648 He-sdB 25069 124 4.73 0.02 0.351 0.9484 0.0391 -10.529 0.033 0.007 0.684 0.029 0.027 165.8 14.9 13.2 0.92 0.09 0.08 +LAMOSTJ052426.53+150514.3 3390739005017699968 sdOB 39607 572 5.32 0.06 0.822 0.4236 0.0748 -11.478 0.035 0.020 0.173 0.037 0.026 66.0 31.7 18.7 0.23 0.12 0.07 +LAMOSTJ052508.76+175713.7 3400347392320018176 sdB 36100 142 5.73 0.03 0.933 0.9905 0.0478 -11.249 0.010 0.003 0.126 0.007 0.006 24.2 2.9 2.6 0.31 0.05 0.04 +LAMOSTJ052750.76+165433.1 3397199529183763072 He-sdO 46075 355 5.61 0.05 1.135 0.7154 0.0439 -11.290 0.010 0.010 0.160 0.011 0.009 103.5 14.4 12.0 0.38 0.07 0.06 +LAMOSTJ052933.93+040719.3 3236488827993523584 He-sdOB 37145 251 5.75 0.08 0.266 0.5531 0.0679 -11.573 0.011 0.007 0.107 0.015 0.012 19.6 6.0 4.3 0.24 0.09 0.06 +LAMOSTJ053033.03+112043.8 3340622921426651648 sdB 30175 258 5.89 0.06 0.776 0.6004 0.0635 -11.411 0.011 0.008 0.143 0.017 0.014 15.2 4.0 3.1 0.58 0.17 0.13 +LAMOSTJ053239.18+433819.8 195587076882426880 sdB 31819 303 5.71 0.08 1.109 0.6081 0.0519 -11.269 0.018 0.011 0.195 0.018 0.015 35.2 7.1 5.6 0.72 0.21 0.16 +LAMOSTJ053307.15+073021.9 3334223901191558784 sdOB 37945 217 5.84 0.04 0.495 1.9994 0.0289 -10.951 0.014 0.006 0.124 0.003 0.003 28.6 1.8 1.7 0.39 0.05 0.04 +LAMOSTJ053321.16+160647.5 3396876131029433472 sdB 35028 193 5.82 0.03 1.084 1.5081 0.0392 -11.077 0.006 0.017 0.123 0.004 0.004 20.3 1.8 1.8 0.36 0.04 0.04 +LAMOSTJ053323.55+212620.3 3403657609512772096 sdO 50546 919 5.60 0.04 1.189 0.6592 0.0778 -11.394 0.029 0.004 0.135 0.018 0.014 107.0 31.5 22.2 0.27 0.08 0.06 +LAMOSTJ053335.87+662115.3 480943256621951360 sdB 30560 238 5.87 0.07 1.000 0.9364 0.0421 -11.246 0.007 0.017 0.134 0.007 0.006 14.1 2.0 1.9 0.49 0.10 0.08 +LAMOSTJ053351.65+191431.0 3400946935393688576 sdB 29089 242 5.40 0.04 0.861 0.6380 0.0467 -11.158 0.046 0.014 0.241 0.019 0.016 37.4 6.4 5.2 0.53 0.11 0.09 +LAMOSTJ053505.93-041255.5 3215662703374964992 sdB 31571 200 5.87 0.05 1.462 0.7884 0.0567 -11.187 0.007 0.016 0.183 0.014 0.012 29.9 5.0 4.2 0.91 0.19 0.15 +LAMOSTJ054217.00+124950.5 3340527779312131584 sdB 31100 390 5.59 0.05 1.245 0.6166 0.0735 -11.352 0.016 0.017 0.160 0.022 0.017 21.6 6.5 4.6 0.37 0.12 0.08 +LAMOSTJ054257.76+391151.2 190164354254168192 sdOB 37164 295 5.96 0.05 0.832 1.2017 0.0320 -11.123 0.006 0.012 0.140 0.004 0.004 33.7 2.6 2.4 0.66 0.09 0.08 +LAMOSTJ054448.13+153040.2 3348217694917419392 sdB 25835 122 4.94 0.02 0.724 0.6602 0.0292 -10.872 0.011 0.004 0.450 0.021 0.019 80.8 7.9 7.0 0.64 0.07 0.06 +LAMOSTJ054456.61+354935.9 3455626713794023680 He-sdO 46268 275 5.74 0.03 1.175 0.8625 0.0344 -11.192 0.006 0.010 0.167 0.007 0.007 114.6 10.1 9.1 0.56 0.07 0.06 +LAMOSTJ054641.31+321942.1 3448218449263806080 sdB 33050 460 5.90 0.13 1.396 0.4873 0.0793 -11.425 0.036 0.014 0.167 0.032 0.023 29.9 12.9 8.0 0.82 0.48 0.29 +LAMOSTJ054704.34+245114.3 3428575497937863808 sdB 32876 284 5.75 0.06 1.245 0.5804 0.0755 -11.278 0.011 0.004 0.201 0.030 0.023 42.5 13.8 9.4 0.83 0.30 0.21 +LAMOSTJ054706.22+400822.5 191727718051389312 sdB 33917 178 6.05 0.03 0.684 1.0531 0.0453 -11.269 0.036 0.017 0.113 0.005 0.005 15.2 2.0 1.9 0.52 0.07 0.06 +LAMOSTJ054711.59+170919.5 3396486324095591040 He-sdOB 39576 383 5.87 0.08 0.785 0.7949 0.0615 -11.442 0.057 0.015 0.101 0.009 0.007 22.4 4.3 3.5 0.28 0.08 0.06 +LAMOSTJ054911.28+163804.8 3348405157352739200 sdB 36214 639 5.86 0.13 0.966 0.5543 0.0955 -11.486 0.043 0.022 0.125 0.026 0.018 24.0 11.4 6.8 0.42 0.26 0.15 +LAMOSTJ055130.20+382842.4 3457951566709510912 sdB 34292 377 5.53 0.05 0.944 0.7548 0.0527 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0.03 +LAMOSTJ055733.97+141217.2 3346893264443563776 sdOB 38848 270 5.62 0.03 0.944 1.1823 0.0357 -11.041 0.086 0.016 0.166 0.006 0.005 56.3 4.2 3.9 0.42 0.05 0.04 +LAMOSTJ055814.18+464025.4 197796403761616256 He-sdO 52829 462 5.78 0.06 0.631 0.4263 0.0752 -11.678 0.016 0.008 0.109 0.023 0.016 83.0 39.6 22.9 0.26 0.13 0.08 +LAMOSTJ055849.80+183110.9 3350560685476251648 sdB 30846 351 5.52 0.06 1.216 0.6587 0.0394 -11.117 0.029 0.016 0.252 0.016 0.014 51.6 7.3 6.2 0.77 0.16 0.13 +LAMOSTJ060000.23+112836.6 3342199204486994048 He-sdOB 40506 148 5.89 0.03 0.759 0.5892 0.0737 -11.417 0.035 0.010 0.144 0.020 0.016 50.0 15.1 10.6 0.59 0.19 0.13 +LAMOSTJ060037.69+364757.4 3456632255835216640 sdB 28167 411 5.62 0.07 0.881 0.9121 0.0456 -11.082 0.018 0.009 0.200 0.011 0.010 22.7 3.1 2.8 0.61 0.13 0.11 +LAMOSTJ060052.82+114548.7 3342214632009904640 sdB 32899 199 5.63 0.03 0.733 0.8193 0.0449 -11.225 0.026 0.014 0.157 0.009 0.008 26.0 3.5 3.0 0.38 0.06 0.05 +LAMOSTJ060101.91+423041.3 960904069540367232 sdOB 37664 182 6.09 0.03 0.638 0.9828 0.0490 -11.229 0.007 0.030 0.133 0.007 0.007 32.2 3.8 3.3 0.80 0.11 0.09 +LAMOSTJ060119.27+142955.0 3345427134406013440 sdB 32872 229 5.78 0.05 1.245 0.6803 0.0459 -11.191 0.033 0.017 0.202 0.015 0.013 42.8 6.6 5.5 0.90 0.18 0.14 +LAMOSTJ060125.51+224446.3 3424487032666787840 sdB 24529 396 5.51 0.07 1.641 0.8311 0.0650 -11.182 0.021 0.017 0.171 0.014 0.013 9.5 2.3 2.0 0.35 0.09 0.07 +LAMOSTJ060453.50+092803.1 3329611552994806272 He-sdO 48397 269 5.69 0.07 0.610 0.6978 0.0352 -11.163 0.007 0.009 0.219 0.012 0.011 236.8 26.2 22.6 0.86 0.18 0.15 +LAMOSTJ060655.95+235233.7 3426156434914782848 sdB 33686 261 5.80 0.05 0.733 0.7578 0.0533 -11.307 0.017 0.006 0.144 0.011 0.010 23.9 4.1 3.4 0.48 0.10 0.08 +LAMOSTJ060916.16+205909.0 3375281653941423360 sdB 28310 280 5.40 0.04 1.841 0.6368 0.0672 -11.181 0.031 0.022 0.219 0.025 0.021 27.6 7.0 5.3 0.44 0.12 0.09 +LAMOSTJ061039.72+075413.7 3328247780618525568 sdB 27896 395 5.57 0.05 0.596 0.9480 0.0325 -11.093 0.019 0.012 0.189 0.007 0.006 19.4 2.3 2.2 0.48 0.07 0.06 +LAMOSTJ061123.00+555215.1 997207297787944064 sdB 30353 215 5.44 0.04 0.335 0.6543 0.0418 -11.308 0.024 0.023 0.166 0.012 0.010 21.1 3.4 2.9 0.28 0.05 0.05 +LAMOSTJ061128.61+485200.6 970006166095484928 sdB 30148 227 5.62 0.04 0.389 0.3633 0.0519 -11.430 0.034 0.008 0.227 0.037 0.028 38.2 13.8 9.1 0.78 0.30 0.19 +LAMOSTJ061205.87+473124.1 969542451362654976 He-sdO 51581 451 5.47 0.05 0.519 0.3094 0.0600 -11.520 0.008 0.011 0.216 0.052 0.035 297.7 159.6 88.9 0.51 0.28 0.16 +LAMOSTJ061255.23+575050.8 999261490450160512 sdB 30365 215 5.47 0.04 0.245 0.6262 0.0522 -11.311 0.023 0.009 0.172 0.016 0.013 22.7 4.6 3.7 0.32 0.07 0.06 +LAMOSTJ061431.94-070752.3 3007619194841792640 sdB 29256 156 5.30 0.03 0.631 1.4107 0.0313 -10.877 0.037 0.009 0.208 0.005 0.005 28.5 2.0 2.0 0.32 0.03 0.03 +LAMOSTJ061432.76+110341.9 3330105641733251840 sdB 33076 140 5.61 0.04 1.035 0.6779 0.0560 -11.320 0.023 0.010 0.156 0.014 0.012 26.3 5.2 4.1 0.36 0.08 0.07 +LAMOSTJ061756.67+184948.6 3373814561832902272 sdB 26954 274 5.10 0.03 0.376 1.5302 0.0288 -10.831 0.006 0.009 0.214 0.005 0.004 21.8 1.9 1.8 0.21 0.03 0.03 +LAMOSTJ061838.26+245623.8 3425819262803882496 sdB 29825 582 5.30 0.11 1.396 0.5725 0.0863 -11.347 0.022 0.015 0.175 0.031 0.023 21.7 8.6 5.7 0.22 0.12 0.07 +LAMOSTJ061916.24+521625.3 995594898345623168 sdB 25821 988 5.44 0.10 0.447 0.8653 0.0343 -11.074 0.018 0.010 0.216 0.009 0.008 18.7 3.7 3.3 0.47 0.13 0.10 +LAMOSTJ062049.36+191828.9 3373940219694568576 sdB 29806 191 5.89 0.03 0.841 1.0560 0.0363 -11.048 0.032 0.012 0.188 0.007 0.007 24.9 2.4 2.2 1.00 0.10 0.09 +LAMOSTJ062239.09+463232.8 968469534172491648 sdB 28031 356 5.39 0.04 0.355 1.0089 0.0356 -11.071 0.013 0.005 0.186 0.007 0.007 19.3 2.3 2.1 0.31 0.04 0.04 +LAMOSTJ062245.22+515046.1 995383482875359744 sdB 33056 294 5.95 0.07 0.351 0.4627 0.0530 -11.472 0.004 0.008 0.162 0.021 0.017 28.0 7.8 5.7 0.85 0.29 0.20 +LAMOSTJ062330.78+330120.6 3439445854003662592 sdOB 40315 435 5.32 0.05 0.750 0.4540 0.0486 -11.415 0.019 0.007 0.188 0.022 0.018 83.5 21.5 15.7 0.27 0.08 0.06 +LAMOSTJ062442.46+282946.5 3433651805682659200 sdOB 34395 198 5.87 0.04 0.537 0.4633 0.0906 -11.643 0.038 0.011 0.108 0.026 0.018 14.7 8.0 4.6 0.32 0.18 0.10 +LAMOSTJ062622.27+040423.7 3131204469305148288 sdB 27397 242 5.67 0.03 0.080 2.9280 0.0435 -10.621 0.016 0.005 0.181 0.003 0.003 16.5 1.6 1.6 0.56 0.05 0.05 +LAMOSTJ062800.46+205057.4 3376012799112785408 He-sdO 70268 1801 5.39 0.07 1.161 0.3399 0.0445 -11.377 0.008 0.014 0.273 0.041 0.032 1635.5 559.9 383.1 0.67 0.25 0.17 +LAMOSTJ062830.43+112018.4 3331029094063986688 He-sdOB 41526 234 5.81 0.11 1.148 0.6153 0.0896 -11.507 0.004 0.014 0.112 0.019 0.014 33.6 12.5 8.1 0.30 0.15 0.10 +LAMOSTJ062836.51+325031.5 3439296187280018432 He-sdOB 43860 258 5.62 0.05 0.462 0.7703 0.0384 -11.211 0.010 0.015 0.177 0.009 0.009 104.5 11.6 10.0 0.48 0.08 0.07 +LAMOSTJ062949.03+222450.4 3376468958998845312 sdB 28290 480 5.59 0.07 0.385 0.6541 0.0389 -11.197 0.046 0.006 0.214 0.014 0.012 26.5 4.2 3.6 0.65 0.15 0.12 +LAMOSTJ063033.77+211928.2 3376057123175008256 sdB 21546 303 5.32 0.04 0.646 0.8602 0.0411 -11.044 0.007 0.014 0.234 0.012 0.011 10.6 1.9 1.8 0.42 0.06 0.06 +LAMOSTJ063359.35+323314.2 3436238720320660224 sdB 28871 304 5.70 0.05 0.327 0.7889 0.0387 -11.161 0.042 0.006 0.194 0.010 0.009 23.4 3.0 2.7 0.69 0.11 0.10 +LAMOSTJ063642.90+115612.7 3352119140132751872 sdO 63106 1969 6.00 0.09 1.496 0.8200 0.0492 -11.319 0.007 0.010 0.130 0.008 0.008 239.4 44.9 37.7 0.61 0.17 0.13 +LAMOSTJ063714.14+422254.1 958032042088084992 sdOB 36835 245 5.89 0.05 0.335 0.5770 0.0872 -11.658 0.015 0.017 0.085 0.015 0.011 11.8 4.8 3.2 0.20 0.09 0.06 +LAMOSTJ063838.63+425653.2 964071899977558784 sdB 29789 511 5.49 0.08 0.367 0.4874 0.0625 -11.350 0.016 0.024 0.204 0.030 0.023 29.4 9.6 6.6 0.47 0.18 0.12 +LAMOSTJ063922.84+304810.1 3435087188048765440 sdB 23931 344 6.08 0.07 0.589 0.5389 0.0859 -11.438 0.035 0.004 0.150 0.028 0.021 6.6 3.1 2.2 0.99 0.46 0.28 +LAMOSTJ064314.84+135755.6 3352890447538648064 sdB 33243 201 5.85 0.04 0.624 1.0353 0.0338 -11.119 0.038 0.004 0.162 0.006 0.005 28.9 2.5 2.4 0.68 0.08 0.08 +LAMOSTJ064508.27+211815.0 3378155777335873664 sdB 26840 606 5.15 0.06 0.422 0.4384 0.0502 -11.333 0.040 0.008 0.235 0.030 0.024 25.7 7.6 5.6 0.29 0.09 0.07 +LAMOSTJ064532.02+114003.1 3351216303643796096 sdB 30293 224 5.98 0.05 0.955 0.6938 0.0648 -11.342 0.022 0.010 0.146 0.015 0.013 16.0 3.7 3.0 0.74 0.19 0.14 +LAMOSTJ064711.24+132213.2 3352595366104656384 sdOB 36364 312 5.83 0.05 0.977 0.7118 0.1165 -11.585 0.005 0.012 0.081 0.016 0.012 10.2 4.6 3.0 0.16 0.08 0.05 +LAMOSTJ064734.86+135011.3 3352835983053282304 sdB 33246 169 6.03 0.03 0.422 0.5559 0.0666 -11.526 0.047 0.006 0.118 0.016 0.013 15.3 4.7 3.4 0.55 0.17 0.12 +LAMOSTJ064918.43+235440.6 3381156177066288768 He-sdB 27120 165 5.10 0.02 0.479 0.4050 0.0545 -11.128 0.026 0.010 0.407 0.063 0.048 80.6 27.1 18.1 0.76 0.26 0.17 +LAMOSTJ064919.17+063320.6 3132895350689573888 sdB 32528 278 4.90 0.05 1.059 0.6646 0.0219 -10.760 0.016 0.007 0.580 0.020 0.019 338.2 26.3 24.0 0.98 0.14 0.12 +LAMOSTJ065027.16+163946.0 3358122782854938112 sdB 30784 230 5.81 0.05 0.188 0.5050 0.0554 -11.429 0.049 0.008 0.164 0.020 0.016 21.6 5.8 4.3 0.63 0.19 0.14 +LAMOSTJ065243.57+401737.6 950627174872167808 He-sdO 65080 495 5.32 0.03 0.180 0.6313 0.0373 -11.209 0.007 0.009 0.218 0.014 0.012 762.3 101.0 85.7 0.36 0.06 0.05 +LAMOSTJ065300.09+342817.7 939393979967463424 sdB 30463 244 5.14 0.04 1.047 0.4886 0.0429 -11.144 0.050 0.013 0.317 0.030 0.025 77.5 15.9 12.2 0.51 0.12 0.09 +LAMOSTJ065446.63+244926.8 3381286602335612416 sdO 52362 550 5.40 0.03 0.111 0.6725 0.0388 -11.188 0.003 0.008 0.214 0.013 0.012 308.6 41.2 34.7 0.42 0.06 0.06 +LAMOSTJ065532.98+220349.6 3378454092881858816 sdO 45839 225 6.07 0.03 0.010 1.7044 0.0475 -11.118 0.010 0.021 0.099 0.003 0.003 38.9 2.8 2.6 0.42 0.04 0.04 +LAMOSTJ065658.95+284457.6 887446174427959040 sdB 31180 255 5.94 0.06 0.251 0.4659 0.0819 -11.515 0.007 0.005 0.145 0.031 0.022 17.9 8.6 5.1 0.67 0.34 0.20 +LAMOSTJ065742.58+051056.6 3129475762151272448 sdOB 34160 313 5.71 0.06 0.741 0.5548 0.0493 -11.420 0.036 0.011 0.150 0.015 0.012 27.6 5.9 4.6 0.42 0.11 0.09 +LAMOSTJ065754.61+121432.1 3160786559070298880 sdO 48269 253 5.78 0.03 0.422 0.6601 0.0517 -11.443 0.031 0.011 0.118 0.010 0.009 68.0 12.3 9.6 0.31 0.06 0.05 +LAMOSTJ065816.72+094343.1 3157967411257049728 sdOB 35676 345 5.23 0.06 0.343 0.7864 0.0364 -10.952 0.011 0.020 0.315 0.015 0.014 144.4 15.5 13.5 0.62 0.11 0.10 +LAMOSTJ070102.95+094135.6 3157919887443293952 sdB 25017 402 5.65 0.05 0.237 0.5514 0.0788 -11.492 0.044 0.005 0.129 0.022 0.016 5.9 2.6 2.0 0.27 0.11 0.07 +LAMOSTJ070256.78+172331.1 3361273433424723712 sdB 31358 165 5.73 0.04 0.180 0.6800 0.0494 -11.323 0.028 0.009 0.154 0.012 0.011 20.7 3.7 3.1 0.47 0.09 0.08 +LAMOSTJ070306.77+193216.0 3364990572999194880 sdOB 40288 417 5.59 0.05 0.172 0.3748 0.0531 -11.477 0.044 0.002 0.197 0.032 0.025 91.7 32.6 21.6 0.55 0.21 0.14 +LAMOSTJ070314.53+363833.5 940053927462368000 sdB 19296 356 5.02 0.06 0.394 0.3078 0.0591 -11.231 0.008 0.009 0.423 0.099 0.068 22.3 11.9 6.8 0.69 0.38 0.22 +LAMOSTJ070514.61+222121.4 3367827072481260416 sdB 27776 345 5.39 0.04 0.114 0.8071 0.0432 -11.190 0.002 0.011 0.178 0.010 0.009 16.9 2.6 2.3 0.28 0.05 0.04 +LAMOSTJ070554.37+335155.2 891442899194878208 sdB 30947 356 5.90 0.10 0.195 0.4420 0.0840 -11.587 0.020 0.010 0.128 0.030 0.020 13.4 7.2 4.2 0.48 0.29 0.17 +LAMOSTJ070633.90+090527.1 3154729899269006336 sdB 28337 277 5.32 0.04 0.324 0.4501 0.0517 -11.394 0.040 0.004 0.198 0.026 0.021 22.8 6.5 4.7 0.30 0.09 0.07 +LAMOSTJ070828.40+442534.8 953141929764017408 He-sdOB 39180 91 5.98 0.01 0.380 0.6622 0.0533 -11.512 0.040 0.011 0.103 0.009 0.008 22.4 4.3 3.5 0.37 0.07 0.06 +LAMOSTJ070905.55+223542.5 3368172319132367104 sdO 47833 642 5.70 0.05 0.065 0.4510 0.0556 -11.588 0.043 0.007 0.126 0.018 0.014 74.7 22.9 15.8 0.29 0.10 0.07 +LAMOSTJ071051.21+051445.0 3140551456311037440 sdOB 36386 524 5.57 0.08 0.525 0.5837 0.0716 -11.535 0.005 0.006 0.111 0.016 0.012 19.4 6.1 4.3 0.17 0.07 0.05 +LAMOSTJ071252.84+423838.0 949617548319629824 sdO 53461 731 5.67 0.04 0.176 0.4885 0.0592 -11.558 0.011 0.007 0.126 0.017 0.014 115.5 34.6 24.2 0.27 0.09 0.06 +LAMOSTJ071305.31+182503.9 3363070035424348800 sdB 26958 317 5.51 0.04 0.302 0.7481 0.0559 -11.285 0.009 0.040 0.154 0.012 0.011 11.2 2.4 2.1 0.28 0.06 0.05 +LAMOSTJ071314.50+173458.6 3360729067791609216 sdB 30291 133 5.74 0.03 0.525 0.5721 0.0581 -11.319 0.054 0.012 0.186 0.021 0.017 26.3 6.3 4.9 0.70 0.17 0.13 +LAMOSTJ071319.65+380739.8 946428174325145856 He-sdOB 41486 174 5.90 0.03 0.295 0.4246 0.0709 -11.731 0.009 0.009 0.097 0.019 0.014 25.0 11.1 6.8 0.27 0.12 0.08 +LAMOSTJ071401.36+693321.7 1109216024779190016 He-sdOB 38576 267 5.58 0.05 0.110 0.3794 0.0445 -11.532 0.005 0.009 0.172 0.023 0.018 58.7 16.8 11.7 0.41 0.13 0.09 +LAMOSTJ071420.01+262850.9 883309884699633280 sdB 31115 209 5.74 0.06 0.299 0.6642 0.0421 -11.184 0.041 0.006 0.218 0.015 0.013 40.1 5.9 4.9 0.96 0.20 0.16 +LAMOSTJ071437.39+264712.0 883333730358019584 sdB 26345 469 5.11 0.06 0.285 0.2938 0.0487 -11.258 0.009 0.012 0.417 0.082 0.059 75.2 33.2 20.4 0.82 0.39 0.23 +LAMOSTJ071856.25+102638.3 3156573539750882944 He-sdOB 32573 189 5.70 0.02 0.207 0.8986 0.0617 -11.391 0.005 0.007 0.100 0.008 0.007 10.1 2.1 1.9 0.18 0.04 0.03 +LAMOSTJ071857.66+073913.2 3154801672464733440 sdOB 45003 731 5.31 0.05 0.232 0.5480 0.0476 -11.360 0.019 0.012 0.172 0.016 0.014 109.1 23.1 18.0 0.22 0.06 0.05 +LAMOSTJ071921.93+051000.4 3140714527629703552 sdOB 37337 234 5.90 0.04 0.385 0.4741 0.0641 -11.498 0.003 0.007 0.149 0.023 0.018 38.6 13.0 8.8 0.64 0.23 0.15 +LAMOSTJ072240.01+091354.5 3155626997678101248 sdO 48776 524 5.94 0.05 0.048 1.9843 0.0532 -10.998 0.009 0.013 0.112 0.004 0.004 64.0 4.8 4.4 0.40 0.06 0.05 +LAMOSTJ072315.72+183456.7 3362524196619239808 He-sdOB 43627 716 5.61 0.20 0.200 0.3547 0.0683 -11.575 0.003 0.007 0.165 0.039 0.027 89.3 47.7 26.8 0.42 0.36 0.19 +LAMOSTJ072327.07+114047.8 3162780553469479040 sdB 30698 325 5.95 0.07 0.248 0.4734 0.0839 -11.582 0.003 0.008 0.123 0.026 0.019 12.0 5.9 3.6 0.49 0.25 0.15 +LAMOSTJ072359.00+042956.6 3139698956841267456 sdB 29917 245 5.44 0.04 0.881 0.5461 0.0432 -11.106 0.066 0.011 0.312 0.027 0.023 69.8 12.8 10.2 0.98 0.20 0.16 +LAMOSTJ072423.96+242126.9 869890070404469760 sdOB 45724 1046 5.76 0.09 0.133 0.6413 0.0440 -11.425 0.004 0.009 0.130 0.010 0.009 66.3 12.1 10.0 0.36 0.10 0.08 +LAMOSTJ072454.93+151650.8 3167124522048560128 sdB 33023 117 5.76 0.02 0.263 0.7276 0.0470 -11.309 0.021 0.005 0.149 0.010 0.009 23.8 3.6 3.1 0.47 0.07 0.06 +LAMOSTJ072535.25+815051.7 1142701823200960512 sdOB 37056 187 5.81 0.03 0.200 0.7912 0.0329 -11.278 0.013 0.005 0.147 0.007 0.006 36.5 3.6 3.2 0.51 0.06 0.06 +LAMOSTJ072542.83+524325.6 986474685615378816 sdB 23668 250 5.10 0.03 0.188 0.8527 0.0453 -11.193 0.006 0.008 0.168 0.010 0.009 7.9 1.7 1.6 0.13 0.03 0.03 +LAMOSTJ072637.25+083330.8 3143342600936696960 sdB 30401 152 5.52 0.03 0.080 0.6685 0.0439 -11.216 0.036 0.006 0.202 0.014 0.012 31.1 4.8 4.0 0.49 0.08 0.07 +LAMOSTJ072738.73+483703.4 976789229421149312 sdOB 36265 278 6.04 0.06 0.437 0.7229 0.0576 -11.438 0.005 0.004 0.112 0.010 0.008 19.4 3.8 3.1 0.50 0.12 0.10 +LAMOSTJ072845.27+132627.0 3163565604772130560 sdB 30442 172 5.65 0.03 0.484 0.5843 0.0493 -11.248 0.013 0.023 0.218 0.020 0.017 36.7 7.2 5.7 0.78 0.16 0.13 +LAMOSTJ072849.83+021400.5 3135810671409226368 sdB 29429 262 5.44 0.04 0.380 0.5093 0.0527 -11.351 0.006 0.010 0.194 0.022 0.018 25.5 6.4 4.8 0.38 0.10 0.08 +LAMOSTJ072949.65-000408.9 3062447063715980672 sdOB 35217 348 5.78 0.06 0.285 0.5755 0.0527 -11.452 0.008 0.009 0.136 0.014 0.012 25.6 5.7 4.4 0.41 0.11 0.08 +LAMOSTJ073215.64+061212.1 3141525486172958336 sdB 28757 327 5.47 0.05 0.153 0.6220 0.0595 -11.351 0.025 0.006 0.159 0.017 0.014 15.5 3.8 3.0 0.27 0.07 0.06 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sdB 31036 210 5.41 0.04 0.422 1.3195 0.0335 -10.873 0.057 0.008 0.223 0.006 0.006 41.4 2.8 2.7 0.47 0.06 0.05 +LAMOSTJ073817.49+134427.9 3164199095268594176 sdB 29404 213 5.62 0.04 0.279 0.4818 0.0806 -11.463 0.007 0.003 0.159 0.032 0.023 16.9 7.6 4.8 0.38 0.18 0.11 +LAMOSTJ073833.37+512844.5 982729822026188928 sdB 30044 165 5.58 0.05 0.209 0.6110 0.0440 -11.254 0.051 0.011 0.202 0.016 0.014 29.9 5.0 4.2 0.57 0.12 0.10 +LAMOSTJ073935.74+564233.2 986254272189606656 sdB 29896 553 5.90 0.11 0.339 0.4180 0.0587 -11.492 0.007 0.008 0.171 0.028 0.021 21.0 7.7 5.2 0.86 0.41 0.26 +LAMOSTJ075139.27+064604.8 3144058245567712512 He-sdOB 40649 139 5.69 0.03 0.024 1.2486 0.0459 -11.034 0.005 0.008 0.164 0.007 0.006 65.7 5.4 4.8 0.48 0.06 0.05 +LAMOSTJ075329.11+232436.2 675213084211549696 sdB 33900 150 5.65 0.03 0.019 1.7590 0.0367 -10.937 0.007 0.033 0.146 0.004 0.004 25.4 1.8 1.8 0.35 0.04 0.03 +LAMOSTJ075922.99+164601.6 667308798199419776 sdOB 41329 470 5.42 0.05 0.075 0.5668 0.0428 -11.185 0.004 0.019 0.256 0.021 0.018 171.2 30.2 24.1 0.63 0.14 0.11 +LAMOSTJ080044.23+180401.9 669097841055847296 sdB 31448 276 5.46 0.05 0.116 0.3405 0.0511 -11.400 0.042 0.007 0.259 0.045 0.034 58.7 22.7 14.4 0.71 0.29 0.18 +LAMOSTJ081351.59+110136.3 648868682531670656 sdB 35789 318 5.39 0.05 0.124 0.3755 0.0489 -11.368 0.015 0.004 0.253 0.038 0.029 94.4 30.4 20.8 0.58 0.20 0.14 +LAMOSTJ082517.99+113106.3 601188910547673728 sdB 34023 569 5.22 0.08 1.189 0.7379 0.0269 -10.917 0.054 0.009 0.360 0.014 0.013 156.0 16.3 14.6 0.79 0.17 0.14 +LAMOSTJ084340.68+020027.2 3078888851357039360 sdOB 42147 553 5.59 0.05 0.221 0.8532 0.0436 -11.119 0.014 0.018 0.198 0.011 0.010 111.5 13.8 12.0 0.56 0.10 0.08 +LAMOSTJ085649.26+170114.6 611587919724027392 sdB 30688 150 5.65 0.03 0.041 1.8709 0.0383 -10.771 0.011 0.013 0.201 0.005 0.004 32.2 2.1 2.0 0.66 0.06 0.06 +LAMOSTJ085851.12+021011.3 577763368640517760 sdO 45501 1372 5.67 0.10 0.029 1.6430 0.0418 -11.041 0.008 0.017 0.123 0.004 0.004 58.4 8.2 7.4 0.26 0.07 0.06 +LAMOSTJ092239.81+270225.2 694109462844643072 sdB 32758 97 5.81 0.02 0.197 2.9732 0.0667 -10.768 0.021 0.025 0.127 0.003 0.003 16.6 1.6 1.6 0.38 0.03 0.03 +LAMOSTJ095932.20+361824.5 795959630108543232 sdB 26050 245 5.14 0.03 0.024 1.6216 0.0429 -10.746 0.005 0.019 0.246 0.007 0.007 25.0 2.2 2.1 0.30 0.04 0.03 +LAMOSTJ101509.38+003300.6 3831905500061334912 sdB 34812 234 6.00 0.05 0.099 0.9408 0.0456 -11.218 0.004 0.015 0.143 0.008 0.007 26.9 3.2 2.9 0.74 0.12 0.10 +LAMOSTJ104652.94+515437.0 837007590331263360 sdOB 42431 815 5.47 0.08 0.035 1.3705 0.0490 -10.812 0.019 0.024 0.250 0.009 0.009 181.3 20.1 17.9 0.67 0.15 0.12 +LAMOSTJ112629.99+212144.7 3978847841769970816 sdB 22985 227 5.09 0.03 0.085 0.2918 0.0459 -11.234 0.003 0.006 0.444 0.083 0.060 49.3 20.2 12.6 0.88 0.37 0.23 +LAMOSTJ112637.08+115958.8 3917380026471466112 sdB 30615 243 5.64 0.05 0.071 0.4661 0.0548 -11.334 0.011 0.005 0.220 0.029 0.023 38.2 11.0 7.8 0.77 0.24 0.17 +LAMOSTJ123451.01+494720.2 1544410045677548288 sdB 30476 238 5.32 0.05 1.072 1.0077 0.0380 -10.784 0.068 0.017 0.349 0.014 0.013 94.3 8.2 7.4 0.93 0.14 0.12 +LAMOSTJ125050.35+161004.4 3934486949931442176 sdB 26675 275 5.56 0.03 0.094 1.1999 0.0393 -11.045 0.012 0.012 0.166 0.006 0.006 12.6 1.7 1.7 0.37 0.04 0.04 +LAMOSTJ131617.95+383153.1 1522950705438939520 sdB 22070 706 5.06 0.11 3.981 8.6436 0.0147 -10.108 0.089 0.026 0.199 0.002 0.002 8.5 1.8 1.7 0.17 0.05 0.04 +LAMOSTJ145806.43+085130.1 1161864283648012160 sdB 22020 170 5.32 0.03 0.086 1.2006 0.0456 -11.024 0.034 0.007 0.174 0.007 0.007 6.4 1.5 1.5 0.23 0.03 0.03 +LAMOSTJ160954.92+171457.1 1198927755470384128 He-sdB 30332 74 4.99 0.02 0.050 1.6149 0.0496 -10.640 0.044 0.014 0.313 0.010 0.009 74.5 5.1 4.6 0.35 0.04 0.03 +LAMOSTJ170303.98+150818.3 4545907052398514432 sdB 30659 307 5.64 0.05 0.327 0.3615 0.0688 -11.541 0.006 0.012 0.176 0.041 0.028 24.6 13.0 7.4 0.50 0.27 0.15 +LAMOSTJ171304.66+245019.5 4571972212486265216 sdB 30787 154 5.96 0.05 0.010 0.4103 0.0643 -11.579 0.015 0.009 0.142 0.026 0.019 16.2 6.6 4.3 0.67 0.29 0.18 +LAMOSTJ171312.35+084820.2 4395447579151491328 sdB 34515 292 5.91 0.08 0.272 0.3840 0.0623 -11.595 0.043 0.007 0.147 0.028 0.020 27.3 11.7 7.2 0.64 0.31 0.19 +LAMOSTJ172009.14+155036.2 4546952309999524096 He-sdOB 43994 300 5.64 0.04 0.148 0.4588 0.0538 -11.614 0.004 0.009 0.118 0.016 0.012 46.6 13.3 9.5 0.22 0.07 0.05 +LAMOSTJ172311.12+175808.9 4553448465214622848 sdB 33591 136 5.89 0.03 0.065 1.0335 0.0335 -11.171 0.012 0.008 0.145 0.005 0.005 24.0 2.2 2.1 0.59 0.06 0.06 +LAMOSTJ172903.19+171937.0 4550175420961718528 sdOB 41110 672 5.76 0.08 0.115 0.3041 0.0456 -11.549 0.007 0.011 0.206 0.036 0.027 108.9 42.4 27.0 0.90 0.40 0.26 +LAMOSTJ173053.22+182506.1 4553345622222014720 sdOB 37986 993 5.64 0.13 1.023 0.3808 0.0567 -11.483 0.114 0.013 0.187 0.033 0.024 65.6 26.4 16.9 0.57 0.31 0.19 +LAMOSTJ173906.41+111748.1 4492802221326659456 sdB 27867 290 5.26 0.03 0.153 1.7380 0.0328 -10.825 0.019 0.008 0.191 0.004 0.004 19.7 1.8 1.8 0.24 0.03 0.03 +LAMOSTJ174246.87+192608.5 4552341394446464000 sdB 31836 294 6.03 0.08 0.292 0.4737 0.0474 -11.477 0.043 0.006 0.155 0.017 0.014 22.2 5.4 4.2 0.95 0.30 0.22 +LAMOSTJ174438.51+205030.8 4552955540409828352 sdB 32677 636 5.53 0.18 0.164 0.4334 0.0428 -11.374 0.015 0.007 0.216 0.024 0.019 47.9 11.9 8.9 0.58 0.34 0.21 +LAMOSTJ174956.05+000636.1 4371689194462064768 sdB 33379 140 5.88 0.03 1.047 1.9840 0.0235 -10.926 0.016 0.011 0.132 0.003 0.003 19.4 1.5 1.5 0.48 0.04 0.04 +LAMOSTJ175802.11+044821.3 4472834712210380032 sdB 28334 345 5.88 0.07 0.468 0.6187 0.0629 -11.297 0.033 0.005 0.180 0.020 0.017 18.7 4.7 3.7 0.90 0.27 0.20 +LAMOSTJ175842.53+044058.2 4472820517339442944 sdB 30617 630 5.63 0.13 0.403 0.4601 0.0763 -11.373 0.028 0.005 0.203 0.040 0.029 32.4 14.4 8.9 0.65 0.38 0.23 +LAMOSTJ175921.93+081247.7 4476146922268993280 sdB 32313 535 5.07 0.08 0.550 0.8665 0.0289 -11.082 0.017 0.007 0.211 0.008 0.007 43.6 4.5 4.2 0.19 0.05 0.04 +LAMOSTJ180007.26+313437.4 4603104815507642752 sdB 26561 369 5.34 0.05 0.104 0.6751 0.0337 -11.195 0.015 0.007 0.210 0.011 0.010 19.6 2.8 2.5 0.35 0.06 0.05 +LAMOSTJ180522.28+151201.2 4498502433203434368 sdB 31280 247 5.61 0.05 0.589 0.5590 0.0673 -11.464 0.054 0.008 0.136 0.019 0.015 15.9 4.9 3.5 0.28 0.09 0.07 +LAMOSTJ180748.64+143027.6 4498196768968750336 sdB 27860 379 5.26 0.04 0.452 0.5200 0.0437 -11.296 0.062 0.011 0.215 0.020 0.017 24.9 5.2 4.1 0.31 0.07 0.06 +LAMOSTJ180933.32+223059.9 4577984720030433536 sdB 27250 262 5.55 0.04 0.202 2.2300 0.0273 -10.727 0.025 0.041 0.187 0.003 0.003 17.3 1.6 1.6 0.45 0.05 0.05 +LAMOSTJ181027.01+141541.0 4497397527098931712 sdB 30976 382 5.46 0.07 0.479 0.4741 0.0527 -11.369 0.818 0.013 0.198 0.025 0.020 32.4 8.9 6.4 0.41 0.14 0.10 +LAMOSTJ181102.81+173759.8 4526224282435916544 He-sdOB 47729 390 6.26 0.05 0.313 0.3867 0.0618 -11.733 0.042 0.013 0.106 0.020 0.015 52.2 21.9 13.5 0.75 0.33 0.20 +LAMOSTJ181147.02+063046.6 4471987980878277120 sdOB 37272 478 5.64 0.07 0.741 0.3420 0.0625 -11.507 0.037 0.013 0.199 0.044 0.031 68.6 34.1 19.8 0.63 0.34 0.20 +LAMOSTJ181209.99+180754.1 4526347084141410432 sdB 29896 314 5.37 0.05 1.148 0.5603 0.0329 -11.081 0.073 0.024 0.312 0.020 0.017 69.6 9.6 8.0 0.83 0.15 0.13 +LAMOSTJ181632.50+345549.2 4605575383775753856 sdO 50712 424 6.05 0.03 0.099 0.4889 0.0441 -11.553 0.043 0.005 0.126 0.013 0.011 94.8 20.0 15.3 0.65 0.15 0.11 +LAMOSTJ181920.24+181042.4 4523666131196149632 sdB 30606 276 5.62 0.06 0.603 0.4004 0.0525 -11.357 0.029 0.008 0.243 0.037 0.028 46.7 15.2 10.3 0.91 0.33 0.22 +LAMOSTJ181932.27+060442.1 4476966603891088640 sdOB 39057 591 5.53 0.07 0.759 0.3676 0.0732 -11.588 0.019 0.008 0.155 0.039 0.026 50.5 28.4 15.6 0.30 0.18 0.10 +LAMOSTJ183652.69+572743.2 2154234138295606272 sdB 29775 217 5.88 0.05 0.204 0.5968 0.0434 -11.471 0.013 0.005 0.125 0.010 0.009 11.1 2.3 2.0 0.44 0.09 0.08 +LAMOSTJ184134.30+411535.9 2110657846788700288 He-sdB 25447 115 4.76 0.01 0.224 0.7597 0.0239 -10.764 0.005 0.009 0.503 0.016 0.015 95.2 6.6 6.1 0.53 0.04 0.04 +LAMOSTJ190301.13+344529.0 2092525388221505792 sdB 28955 185 5.58 0.02 0.200 0.5026 0.0355 -11.292 0.056 0.006 0.225 0.017 0.015 32.0 5.3 4.4 0.70 0.12 0.10 +LAMOSTJ192045.41+371018.8 2051051736604520960 sdOB 35245 505 5.65 0.08 0.272 0.3976 0.0736 -11.695 0.018 0.003 0.112 0.025 0.017 17.4 8.9 5.2 0.21 0.12 0.07 +LAMOSTJ193408.06+350003.2 2048109069842534912 sdB 35607 198 5.69 0.04 0.260 0.7685 0.0297 -11.304 0.042 0.007 0.143 0.006 0.006 29.7 2.9 2.6 0.37 0.05 0.05 +LAMOSTJ193435.77+362649.5 2048519393833049088 sdOB 35209 658 5.79 0.10 1.109 0.3387 0.0630 -11.588 0.039 0.017 0.163 0.037 0.026 36.5 18.9 10.9 0.60 0.36 0.21 +LAMOSTJ193527.95+354358.8 2048434490916786176 sdB 31703 238 5.71 0.05 0.452 0.8145 0.0369 -11.277 0.036 0.009 0.142 0.007 0.006 18.4 2.3 2.2 0.38 0.06 0.06 +LAMOSTJ193756.87+360625.8 2048280009543018112 sdB 29042 273 5.90 0.07 0.151 1.1777 0.0283 -11.208 0.045 0.004 0.116 0.003 0.003 8.6 1.5 1.5 0.39 0.07 0.06 +LAMOSTJ200134.43+443427.5 2076135724307679872 sdOB 36457 198 5.58 0.04 0.582 0.6180 0.0265 -11.269 0.026 0.006 0.192 0.009 0.008 58.6 5.7 5.0 0.51 0.07 0.06 +LAMOSTJ202453.09+073419.1 1751972311716626048 sdB 30832 243 5.80 0.07 0.556 0.3577 0.0673 -11.510 0.857 0.009 0.191 0.044 0.030 29.5 15.1 8.7 0.84 0.47 0.27 +LAMOSTJ202610.56+055413.9 4246471312729900544 He-sdO 48400 392 5.79 0.05 0.116 0.4951 0.0492 -11.473 0.008 0.012 0.151 0.017 0.014 111.8 26.3 19.4 0.51 0.14 0.10 +LAMOSTJ210148.29+151022.6 1763211279056787968 sdB 29513 482 5.50 0.08 0.295 0.6213 0.0462 -11.346 0.020 0.008 0.160 0.013 0.011 17.5 3.5 2.9 0.30 0.08 0.07 +LAMOSTJ210253.23+355845.1 1868262502632099584 sdOB 37085 745 5.93 0.15 0.556 0.3853 0.0727 -11.716 0.546 0.011 0.110 0.026 0.018 20.6 11.0 6.3 0.38 0.27 0.15 +LAMOSTJ210926.94+370822.8 1868767831308190976 sdO 50644 425 5.80 0.04 0.245 0.7334 0.0317 -11.387 0.043 0.005 0.124 0.006 0.005 90.3 9.0 8.0 0.35 0.05 0.05 +LAMOSTJ210929.38+131646.2 1758993857393963776 sdB 28142 213 5.76 0.03 0.351 0.7634 0.0380 -11.180 0.041 0.004 0.191 0.010 0.009 20.6 2.7 2.4 0.77 0.10 0.09 +LAMOSTJ211000.76+152912.8 1760662130066900352 He-sdOB 47935 384 5.96 0.06 0.243 0.4500 0.0607 -11.603 0.011 0.008 0.123 0.019 0.015 71.6 24.1 16.1 0.50 0.19 0.13 +LAMOSTJ211531.48+123957.6 1746789866736764800 sdB 30265 113 5.62 0.03 0.069 0.4664 0.0473 -11.386 0.016 0.022 0.196 0.022 0.018 28.8 7.0 5.2 0.58 0.15 0.11 +LAMOSTJ211832.42+233417.4 1792255325381143040 He-sdO 44729 194 5.62 0.03 0.272 0.5226 0.0316 -11.245 0.016 0.012 0.241 0.016 0.014 209.0 27.8 23.2 0.89 0.14 0.11 +LAMOSTJ212205.57+214111.5 1790728894004387712 sdB 27345 321 5.40 0.04 0.372 0.9229 0.0577 -11.148 0.017 0.008 0.171 0.012 0.010 14.6 2.6 2.3 0.27 0.05 0.04 +LAMOSTJ212224.98+175144.6 1785228484006179456 sdOB 40075 735 5.08 0.06 1.531 0.7152 0.0229 -10.898 0.047 0.012 0.387 0.013 0.012 347.7 35.2 32.3 0.66 0.11 0.10 +LAMOSTJ212426.05+364458.4 1963732715013489280 sdB 25773 768 5.83 0.09 0.575 0.4451 0.0779 -11.625 0.002 0.012 0.117 0.025 0.018 5.4 3.0 2.1 0.34 0.19 0.11 +LAMOSTJ212608.14+024533.9 2691867011851791744 sdB 32556 264 5.77 0.06 0.111 0.5290 0.0618 -11.417 0.028 0.009 0.160 0.021 0.017 25.9 7.5 5.4 0.55 0.18 0.13 +LAMOSTJ212649.47+154536.8 1783628003096502144 sdB 35832 235 6.03 0.04 0.275 0.3704 0.0738 -11.645 0.043 0.007 0.135 0.034 0.022 27.1 15.3 8.4 0.72 0.41 0.22 +LAMOSTJ212747.81+023105.8 2691890784495579392 sdOB 33686 229 5.72 0.06 0.176 0.5251 0.0855 -11.614 0.011 0.005 0.103 0.020 0.014 12.2 5.3 3.5 0.20 0.10 0.06 +LAMOSTJ212920.56+295806.8 1850084998438797312 sdOB 35665 89 6.11 0.02 0.437 1.7159 0.0252 -11.026 0.027 0.008 0.121 0.003 0.003 21.4 1.6 1.6 0.69 0.04 0.04 +LAMOSTJ213129.05+195157.0 1787066145893240576 sdOB 41294 246 6.14 0.03 0.040 2.6360 0.0362 -10.973 0.009 0.015 0.090 0.002 0.002 21.0 1.6 1.6 0.41 0.04 0.04 +LAMOSTJ213818.52+342105.6 1950263255195349888 sdB 30844 296 5.33 0.04 0.525 0.9600 0.0259 -11.064 0.033 0.012 0.199 0.006 0.006 32.1 2.6 2.5 0.31 0.04 0.04 +LAMOSTJ213827.14+461132.7 1977291346957976320 sdB 33458 180 5.62 0.04 0.692 0.6251 0.0338 -11.358 0.022 0.008 0.156 0.009 0.008 27.2 3.6 3.1 0.37 0.06 0.05 +LAMOSTJ213920.03+393248.8 1953965379566626816 He-sdO 48996 369 5.77 0.03 0.692 0.8576 0.0266 -11.185 0.039 0.011 0.168 0.006 0.005 146.5 10.6 9.7 0.61 0.06 0.06 +LAMOSTJ214106.76+252829.9 1797986937760585600 He-sdO 44022 280 5.76 0.05 0.168 0.9367 0.0342 -11.159 0.005 0.009 0.165 0.006 0.006 91.3 7.5 6.8 0.57 0.09 0.07 +LAMOSTJ214242.40+330452.8 1946937541760735872 sdOB 36926 125 5.92 0.02 0.302 1.0027 0.0324 -11.196 0.006 0.010 0.141 0.005 0.005 33.3 2.7 2.5 0.61 0.05 0.05 +LAMOSTJ214600.31+372119.7 1952553606634620928 He-sdO 53123 459 5.93 0.06 0.955 0.9514 0.0215 -11.140 0.007 0.014 0.169 0.004 0.004 204.0 12.0 11.2 0.89 0.14 0.12 +LAMOSTJ214620.68+224503.7 1794184349811337728 sdB 31289 361 5.76 0.09 0.417 0.5481 0.0497 -11.409 0.009 0.010 0.158 0.016 0.013 21.4 4.8 3.8 0.53 0.17 0.13 +LAMOSTJ215529.65+044217.8 2696716270447621632 sdOB 36880 811 5.21 0.11 1.514 0.4273 0.0501 -11.099 0.088 0.011 0.407 0.053 0.043 274.7 81.8 58.4 0.98 0.42 0.28 +LAMOSTJ215956.51+141804.8 1768547964899107584 He-sdOB 35704 93 5.98 0.02 0.141 0.6272 0.0628 -11.492 0.006 0.007 0.114 0.013 0.010 18.9 4.6 3.6 0.45 0.11 0.08 +LAMOSTJ221002.71+250358.2 1879544900675463552 sdB 21420 129 5.26 0.02 0.197 2.3685 0.0331 -10.632 0.007 0.004 0.218 0.004 0.004 9.0 1.4 1.4 0.32 0.03 0.03 +LAMOSTJ221106.31+513832.4 2004114070560436736 sdB 33090 780 5.40 0.08 0.556 0.4670 0.0294 -11.209 0.009 0.012 0.294 0.020 0.017 92.8 16.1 13.4 0.79 0.20 0.16 +LAMOSTJ221518.33+163703.5 1775141422597602176 sdO 50882 388 5.77 0.04 0.080 0.3693 0.0721 -11.746 0.009 0.007 0.107 0.026 0.018 69.2 37.5 20.9 0.25 0.14 0.08 +LAMOSTJ221607.18+150338.5 2735467282163538944 sdOB 36410 188 5.91 0.03 0.127 0.4824 0.0909 -11.649 0.005 0.006 0.103 0.024 0.016 16.8 8.8 5.1 0.32 0.17 0.10 +LAMOSTJ222216.98+265616.6 1881671180067646080 sdB 28588 440 5.41 0.06 0.776 0.3864 0.0610 -11.391 0.042 0.021 0.222 0.041 0.030 29.6 12.3 7.8 0.47 0.21 0.13 +LAMOSTJ222217.89+273519.9 1881776668761026688 sdO 63364 1052 5.46 0.04 0.944 0.5195 0.0551 -11.286 0.096 0.020 0.212 0.025 0.020 650.9 169.7 124.5 0.47 0.13 0.10 +LAMOSTJ224021.21+120533.1 2729936846049609728 sdB 31381 245 5.50 0.05 0.050 0.4508 0.0812 -11.575 0.014 0.007 0.130 0.029 0.020 14.8 7.3 4.4 0.20 0.10 0.06 +LAMOSTJ230919.30+365359.3 1915148289773812352 sdOB 33190 292 5.82 0.06 0.266 0.5276 0.0545 -11.483 0.011 0.011 0.139 0.016 0.013 20.9 5.3 4.0 0.46 0.14 0.10 +LAMOSTJ232056.49+342343.1 1912906626082386304 sdOB 38266 152 6.03 0.03 0.380 0.7715 0.0337 -11.313 0.005 0.006 0.140 0.007 0.006 37.7 3.8 3.4 0.77 0.09 0.08 +LAMOSTJ232326.23+410613.3 1924304197976603008 sdB 30528 228 5.65 0.06 0.468 0.3381 0.0574 -11.534 0.034 0.010 0.191 0.040 0.027 28.6 13.1 7.8 0.60 0.29 0.18 +LAMOSTJ232336.15+451303.8 1937879932466496896 sdB 26622 370 5.99 0.05 0.589 0.5112 0.0647 -11.447 0.039 0.005 0.155 0.022 0.017 10.8 3.7 2.7 0.85 0.29 0.20 +LAMOSTJ232529.33+413106.2 1923590271333313792 sdOB 38367 202 5.67 0.03 0.437 0.6031 0.0453 -11.491 0.032 0.011 0.119 0.010 0.008 27.5 4.9 4.0 0.24 0.05 0.04 +LAMOSTJ232922.64+321359.3 2872454748672529280 sdB 30127 257 5.28 0.05 0.473 0.3954 0.0678 -11.533 0.042 0.012 0.161 0.033 0.023 19.2 8.8 5.4 0.18 0.09 0.06 +LAMOSTJ233305.19+412812.4 1923812200882866560 sdB 24886 706 5.57 0.09 0.367 0.4773 0.0926 -11.625 0.043 0.012 0.110 0.026 0.018 4.2 2.7 1.9 0.17 0.10 0.06 +LAMOSTJ233445.42+510016.9 1944738965178800384 sdOB 40008 348 5.68 0.04 0.457 0.4598 0.0383 -11.426 0.032 0.006 0.180 0.016 0.014 74.9 14.5 11.4 0.57 0.13 0.10 +LAMOSTJ233641.26+313200.5 2871378846483069184 sdB 33840 208 5.90 0.04 0.724 0.4286 0.0631 -11.503 0.033 0.011 0.159 0.028 0.020 29.7 11.3 7.2 0.73 0.29 0.19 +LAMOSTJ233843.59+004258.5 2645931305829355264 sdB 26032 457 5.28 0.06 0.347 0.4352 0.0605 -11.290 0.008 0.010 0.261 0.042 0.032 28.1 10.1 6.8 0.48 0.18 0.12 +LB400 661156102927711104 sdB 24199 125 5.27 0.02 0.141 1.0432 0.0306 -10.749 0.008 0.024 0.379 0.012 0.011 44.3 3.2 3.0 0.98 0.08 0.07 +NGC7094 1770058865674512896 He-sdOB 115000 5000 5.60 0.10 0.193 0.6263 0.0336 -11.143 0.033 0.010 0.254 0.015 0.013 10168.0 2272.1 1894.2 0.94 0.27 0.21 +O11J181948+332209 4592825172063276288 sdB 29683 255 5.51 0.04 0.151 0.2765 0.0387 -11.458 0.006 0.007 0.279 0.045 0.034 54.2 19.1 12.6 0.92 0.34 0.22 +O11J182055+331847 4593184093889740672 sdB 26413 461 5.70 0.06 0.034 0.3783 0.0560 -11.556 0.024 0.006 0.162 0.028 0.021 11.5 4.6 3.2 0.48 0.20 0.13 +O11J182637+343726 2095370374556456192 He-sdOB 35367 163 6.08 0.04 0.085 0.8226 0.0320 -11.391 0.005 0.007 0.110 0.005 0.005 17.0 2.0 1.9 0.53 0.07 0.06 +PB166 1553487166999658112 He-sdOB 24219 72 5.18 0.02 0.166 1.4588 0.0318 -10.571 0.017 0.029 0.419 0.009 0.009 54.2 2.9 2.8 0.97 0.07 0.06 +PB5018 2679677791586720896 sdB 32002 219 5.69 0.05 0.556 0.5130 0.0730 -11.414 0.019 0.010 0.167 0.028 0.021 26.3 9.5 6.3 0.50 0.19 0.13 +PG0001+275 2854091981071865344 sdB 25400 500 5.30 0.10 0.088 1.7692 0.0329 -10.832 0.029 0.010 0.184 0.004 0.004 12.7 1.8 1.8 0.25 0.07 0.06 +PG0004+133 2767874292175410560 sdB 30322 142 5.47 0.03 0.525 2.0898 0.0285 -10.717 0.011 0.041 0.207 0.003 0.003 32.6 1.8 1.8 0.46 0.04 0.04 +PG0006+120 2766032919436757504 sdB 33112 136 5.94 0.03 0.389 1.1829 0.0489 -11.100 0.006 0.011 0.149 0.007 0.006 24.0 2.6 2.4 0.71 0.08 0.07 +PG0009+191 2797293512483062912 sdB 28950 196 5.53 0.03 0.138 0.8772 0.0362 -11.101 0.007 0.026 0.200 0.009 0.008 25.3 2.7 2.5 0.50 0.06 0.05 +PG0011+283 2859984160805522176 sdB 24938 298 5.35 0.04 0.091 2.6612 0.0463 -10.646 0.027 0.008 0.187 0.004 0.004 12.1 1.6 1.6 0.29 0.04 0.03 +PG0016+151 2792535543417139712 He-sdO 43827 2000 6.30 0.20 0.098 0.4448 0.0869 -11.655 0.007 0.010 0.110 0.027 0.018 40.6 23.8 13.6 0.90 0.79 0.40 +PG0022+087 2750667003920099200 sdB 30221 254 5.39 0.05 0.166 0.5914 0.0543 -11.300 0.012 0.009 0.188 0.019 0.016 26.4 5.8 4.5 0.32 0.08 0.06 +PG0023+298 2859002017748155776 He-sdOB 35215 243 5.33 0.04 1.718 0.7788 0.0327 -10.971 0.105 0.024 0.289 0.013 0.012 115.6 10.9 9.6 0.65 0.09 0.08 +PG0026+047 2554910434747250944 sdB 35355 173 5.70 0.02 0.067 0.7354 0.0537 -11.260 0.017 0.006 0.164 0.013 0.011 37.8 6.4 5.2 0.49 0.09 0.07 +PG0033+266 2809421366255514112 sdB 28583 226 5.65 0.03 0.110 1.1590 0.0398 -11.016 0.006 0.004 0.184 0.007 0.006 20.4 2.1 2.0 0.55 0.06 0.06 +PG0046+207 2801448085887897216 sdB 27520 500 5.55 0.07 0.093 0.9486 0.0371 -11.077 0.018 0.009 0.195 0.008 0.008 19.6 2.6 2.4 0.49 0.10 0.08 +PG0046+247 2805016413436835200 sdB 32776 675 5.59 0.14 0.166 0.5229 0.0793 -11.562 0.015 0.008 0.116 0.021 0.015 14.0 5.8 3.8 0.20 0.11 0.07 +PG0048+004 2537182630815412736 sdOB 38500 300 5.83 0.07 0.059 0.5851 0.0564 -11.481 0.007 0.010 0.125 0.013 0.011 30.9 7.2 5.4 0.39 0.12 0.09 +PG0055+016 2537690089791382656 sdB 34901 155 5.75 0.01 0.457 0.7864 0.0502 -11.216 0.051 0.053 0.159 0.011 0.010 33.5 4.9 4.2 0.52 0.08 0.06 +PG0101+039 2551900379931546240 sdB 27500 500 5.53 0.07 0.046 2.9888 0.0464 -10.584 0.006 0.036 0.194 0.004 0.004 19.3 2.1 2.0 0.46 0.09 0.07 +PG0112+142 2590919234398332544 sdOB 40948 2000 5.18 0.20 0.229 0.3802 0.0502 -11.340 0.023 0.007 0.265 0.040 0.031 178.2 72.3 48.6 0.39 0.28 0.16 +PG0113+259 294818409307323904 He-sdO 54410 4750 5.89 0.24 0.221 0.8294 0.0401 -11.251 0.008 0.013 0.150 0.008 0.007 177.9 74.2 55.6 0.64 0.48 0.27 +PG0123+159 2592234628262141312 sdB 29716 279 5.29 0.04 0.263 1.0762 0.0388 -11.050 0.006 0.008 0.184 0.007 0.007 23.7 2.5 2.3 0.24 0.04 0.03 +PG0133+114 2585744516065582848 sdB 30073 201 5.70 0.04 0.164 3.1957 0.0774 -10.633 0.006 0.008 0.161 0.004 0.004 19.1 1.8 1.7 0.48 0.06 0.05 +PG0142+148 2588387849393475840 sdB 26200 1300 5.10 0.20 0.186 1.3257 0.0374 -10.931 0.006 0.009 0.197 0.006 0.006 16.3 3.9 3.4 0.18 0.11 0.07 +PG0154+204 97013488627139328 sdOB 36462 206 5.86 0.04 0.266 0.6137 0.0469 -11.314 0.005 0.004 0.175 0.015 0.013 48.6 8.5 6.9 0.81 0.16 0.13 +PG0207+005 2507305841871897216 sdB 31414 500 5.83 0.05 0.069 0.6605 0.0543 -11.325 0.005 0.006 0.159 0.014 0.012 22.1 4.6 3.8 0.62 0.14 0.11 +PG0208+015 2514184283536110720 He-sdO 43823 217 5.77 0.05 0.062 1.1104 0.0418 -11.094 0.006 0.013 0.161 0.007 0.006 85.7 7.3 6.4 0.56 0.09 0.07 +PG0209+017 2514278566658235776 sdB 32161 138 6.03 0.03 0.012 1.3453 0.0434 -11.079 0.009 0.013 0.138 0.005 0.005 18.2 1.9 1.8 0.74 0.08 0.07 +PG0212+143 75811331030771200 sdB 25400 1300 5.00 0.20 0.363 0.7823 0.0391 -11.042 0.006 0.007 0.256 0.014 0.012 24.5 6.3 5.3 0.24 0.15 0.09 +PG0212+230 101096662495962240 sdB 27540 148 5.72 0.02 0.302 0.8809 0.0608 -11.247 0.014 0.004 0.142 0.011 0.009 10.4 2.1 1.9 0.39 0.07 0.06 +PG0216+246 102803104542235008 He-sdOB 41200 105 5.87 0.04 0.240 0.3957 0.0686 -11.566 0.006 0.012 0.152 0.032 0.022 59.9 27.7 16.2 0.63 0.30 0.18 +PG0221+217 99836961472298752 He-sdOB 37726 133 5.87 0.03 0.394 0.7955 0.0441 -11.369 0.009 0.021 0.119 0.007 0.007 26.0 3.4 3.0 0.39 0.06 0.05 +PG0240+046 6052403489630720 He-sdOB 36414 223 5.79 0.02 0.053 1.4884 0.0483 -11.104 0.005 0.017 0.118 0.004 0.004 21.9 2.1 2.0 0.31 0.03 0.03 +PG0242+132 31918414533148928 sdB 32755 211 5.40 0.04 0.519 1.4528 0.0333 -10.801 0.011 0.009 0.240 0.006 0.006 59.8 3.5 3.3 0.53 0.06 0.06 +PG0250+189 84006403509432192 sdB 26100 1500 5.81 0.15 0.575 1.9683 0.0285 -10.842 0.044 0.010 0.161 0.003 0.003 10.8 3.1 2.7 0.61 0.26 0.18 +PG0258+184 35928500943041152 sdB 28092 0 5.52 0.00 1.161 0.6607 0.0594 -11.054 0.043 0.018 0.286 0.028 0.023 45.6 9.6 7.3 0.99 0.21 0.16 +PG0305+152 31265029748469120 sdB 54318 2449 5.56 0.12 0.427 1.1406 0.0354 -11.165 0.010 0.013 0.133 0.005 0.004 138.7 28.2 24.4 0.24 0.08 0.06 +PG0314+180 56105192148111616 sdO 67208 6011 5.18 0.19 0.204 1.1716 0.0372 -11.004 0.009 0.011 0.187 0.006 0.006 644.5 267.2 203.0 0.19 0.11 0.07 +PG0319+054 9132341717393792 sdB 30700 500 5.74 0.06 0.638 1.1951 0.0421 -11.131 0.008 0.011 0.140 0.005 0.005 15.6 2.1 2.0 0.39 0.07 0.06 +PG0349+094 3302502234815943296 sdB 23385 217 5.35 0.03 0.427 0.7958 0.0406 -11.154 0.005 0.004 0.195 0.011 0.010 10.2 1.9 1.7 0.31 0.05 0.04 +PG0815+405 909317797165729024 sdB 23067 172 5.55 0.03 0.162 0.8961 0.0410 -11.069 0.009 0.004 0.211 0.010 0.009 11.3 1.8 1.7 0.58 0.07 0.07 +PG0823+465 930163614211158528 sdB 29900 1000 5.75 0.15 0.053 1.0047 0.0415 -11.094 0.014 0.015 0.179 0.008 0.007 22.9 4.1 3.6 0.66 0.28 0.20 +PG0826+480 930769616916994048 sdB 25300 600 5.38 0.06 0.068 0.4869 0.0538 -11.370 0.021 0.009 0.194 0.024 0.019 13.9 4.1 3.2 0.33 0.10 0.08 +PG0833+211 664631178147534720 sdB 33427 225 6.13 0.05 0.061 0.5478 0.0878 -11.494 0.006 0.007 0.130 0.025 0.018 19.0 8.0 5.1 0.84 0.37 0.23 +PG0837+401 911573758803336960 sdB 31426 177 5.99 0.04 0.135 0.7404 0.0438 -11.267 0.008 0.008 0.162 0.010 0.009 23.0 3.3 2.9 0.94 0.16 0.13 +PG0838+132 603097422215268736 He-sdO 47660 3710 5.68 0.29 0.070 0.7819 0.0375 -11.092 0.006 0.018 0.229 0.012 0.011 244.1 90.4 69.8 0.92 0.88 0.45 +PG0839+336 710337051880367616 sdB 29483 303 5.59 0.05 0.127 0.7268 0.0413 -11.132 0.020 0.010 0.223 0.013 0.012 33.7 4.6 4.0 0.71 0.13 0.11 +PG0844+232 689367475352913280 sdO 56847 6000 5.60 0.20 0.122 0.6117 0.0552 -11.435 0.043 0.006 0.133 0.013 0.011 165.8 92.2 62.6 0.26 0.17 0.10 +PG0848+249 690001549964561792 sdO 70000 5940 5.56 0.10 0.389 1.0034 0.0643 -11.171 0.062 0.014 0.145 0.010 0.009 454.5 191.4 142.0 0.28 0.09 0.07 +PG0849+319 706760168755893888 sdB 28900 1000 5.37 0.15 0.016 0.8895 0.0493 -11.034 0.027 0.006 0.230 0.014 0.012 33.1 6.5 5.6 0.45 0.20 0.14 +PG0850+170 611684298790301568 sdB 27100 1000 5.37 0.15 0.040 1.2519 0.0467 -10.963 0.015 0.008 0.193 0.008 0.007 18.0 3.5 3.1 0.32 0.14 0.10 +PG0854+385 719606175420853888 sdB 31725 967 5.62 0.14 0.080 0.4696 0.0518 -11.349 0.010 0.003 0.211 0.026 0.021 40.7 12.1 8.9 0.68 0.33 0.22 +PG0856+121 604794342318395520 sdB 26248 298 5.80 0.04 0.068 1.8631 0.0338 -10.843 0.016 0.006 0.170 0.004 0.004 12.4 1.6 1.6 0.67 0.07 0.07 +PG0901+309 711773838699959296 sdOB 36385 138 5.83 0.03 0.062 0.7844 0.0546 -11.319 0.011 0.008 0.136 0.010 0.009 28.9 4.7 3.9 0.45 0.08 0.07 +PG0902+057 580372234855320064 He-sdOB 42550 87 5.94 0.04 0.112 1.2267 0.0529 -11.148 0.006 0.029 0.129 0.006 0.006 48.9 4.8 4.2 0.53 0.07 0.07 +PG0902+124 604474251290699776 sdB 28050 840 5.50 0.15 0.030 0.8874 0.0392 -11.102 0.014 0.020 0.197 0.009 0.009 21.7 3.7 3.3 0.45 0.19 0.14 +PG0905+627 1043176057879022336 sdO 48000 4900 5.68 0.17 0.087 0.3176 0.0485 -11.631 0.019 0.006 0.164 0.029 0.022 128.5 84.6 51.9 0.47 0.31 0.18 +PG0906+597 1039246845702047360 sdO 69329 2422 6.50 0.11 0.024 1.3258 0.0490 -11.493 0.011 0.009 0.054 0.003 0.003 59.6 10.2 8.9 0.33 0.10 0.08 +PG0907+123 604238612204857088 sdB 26200 900 5.30 0.10 0.123 1.1489 0.0350 -10.948 0.016 0.014 0.218 0.007 0.007 20.1 3.5 3.1 0.35 0.09 0.08 +PG0909+164 607898538520616704 sdB 35300 500 5.33 0.05 0.058 0.8689 0.0430 -10.997 0.012 0.019 0.257 0.013 0.012 91.8 11.2 9.8 0.51 0.09 0.08 +PG0909+276 695059062934110592 sdOB 35500 500 6.09 0.05 0.058 3.6238 0.0630 -10.746 0.007 0.006 0.109 0.003 0.003 17.0 1.8 1.8 0.53 0.07 0.06 +PG0911+042 578986163009656320 sdB 30268 233 5.66 0.05 0.124 0.5274 0.0564 -11.283 0.006 0.010 0.219 0.026 0.021 36.1 9.3 6.8 0.80 0.23 0.17 +PG0912+189 635660764741010304 sdB 28739 422 5.49 0.05 0.036 0.3601 0.0545 -11.325 0.017 0.009 0.291 0.052 0.038 52.0 20.4 13.0 0.96 0.40 0.25 +PG0914-037 5758956484239854336 He-sdO 45136 1000 5.79 0.10 0.086 0.4363 0.0502 -11.398 0.007 0.013 0.204 0.026 0.021 154.7 45.3 32.3 0.94 0.37 0.26 +PG0918+029 3845583703883921920 sdB 32369 173 5.81 0.03 0.044 2.1328 0.0484 -10.906 0.010 0.008 0.129 0.004 0.003 16.4 1.6 1.6 0.39 0.04 0.04 +PG0920+029 3845526597998730368 sdB 29100 440 5.41 0.09 0.104 0.9174 0.0453 -11.064 0.007 0.009 0.209 0.011 0.010 28.1 3.8 3.4 0.41 0.11 0.09 +PG0920+297 695726844449223040 sdB 33057 110 6.20 0.03 0.055 1.3063 0.0519 -11.166 0.008 0.020 0.116 0.005 0.005 14.5 1.9 1.8 0.78 0.09 0.08 +PG0921+311 700362419831670016 He-sdO 40830 160 5.84 0.15 0.016 0.8259 0.0513 -11.267 0.004 0.007 0.145 0.010 0.009 52.7 7.3 6.2 0.54 0.24 0.17 +PG0926+065 586043309672965888 sdB 26060 680 5.45 0.08 0.038 1.1569 0.0347 -10.993 0.008 0.023 0.196 0.006 0.006 16.0 2.5 2.3 0.40 0.09 0.07 +PG0927+311 697406932576439680 sdB 30548 140 5.89 0.03 0.106 0.9290 0.0471 -11.158 0.004 0.005 0.166 0.009 0.008 21.5 2.8 2.5 0.78 0.10 0.09 +PG0928+031 3844661557225496064 sdB 30000 600 5.67 0.18 0.211 0.9370 0.0407 -11.176 0.013 0.013 0.158 0.007 0.007 18.2 2.7 2.5 0.43 0.22 0.15 +PG0932+314 697707958245002880 sdB 35134 252 5.66 0.04 0.017 0.4789 0.0630 -11.407 0.008 0.010 0.182 0.027 0.021 45.1 14.7 10.0 0.55 0.19 0.13 +PG0934+186 633011250955383168 sdB 35855 112 5.76 0.02 0.055 1.5666 0.0467 -10.911 0.012 0.016 0.174 0.006 0.005 45.2 3.2 3.0 0.64 0.05 0.05 +PG0934+553 1021648582279419648 sdOB 47202 781 5.43 0.09 0.272 2.2647 0.0456 -10.719 0.101 0.009 0.185 0.004 0.004 152.8 12.3 11.5 0.34 0.08 0.07 +PG0935-038 3824642199263291136 sdB 34303 160 5.76 0.03 0.295 0.7751 0.0537 -11.160 0.076 0.011 0.194 0.015 0.013 46.9 7.4 6.0 0.79 0.14 0.11 +PG0940+068 3853346290335592320 sdB 28069 254 5.33 0.04 0.150 1.2462 0.0429 -10.886 0.033 0.010 0.229 0.008 0.008 29.3 2.8 2.6 0.41 0.05 0.05 +PG0940+171 620566974057395840 sdB 27982 1098 5.52 0.16 0.380 0.3672 0.0575 -11.372 0.033 0.010 0.252 0.046 0.034 35.1 15.7 9.9 0.78 0.50 0.29 +PG0941+280 648029239761019776 sdB 29400 500 5.43 0.05 0.017 1.5588 0.0439 -10.876 0.014 0.022 0.189 0.006 0.006 23.9 2.6 2.5 0.35 0.05 0.05 +PG0942-029 3826259821385575296 sdOB 43221 247 6.24 0.02 0.039 1.9084 0.0442 -11.129 0.009 0.010 0.087 0.003 0.003 23.5 1.9 1.8 0.48 0.04 0.04 +PG0944+275 647193232966817280 sdB 32501 205 5.92 0.05 0.087 0.4529 0.0695 -11.522 0.015 0.005 0.146 0.027 0.019 21.5 8.6 5.5 0.65 0.27 0.18 +PG0948+041 3849462024992532608 sdB 29800 300 5.48 0.04 0.407 0.4763 0.0536 -11.306 0.054 0.019 0.222 0.028 0.023 35.0 9.6 7.0 0.55 0.16 0.11 +PG0948+187 627130616093753600 sdOB 35513 164 6.04 0.04 0.347 0.6382 0.0838 -11.429 0.073 0.014 0.126 0.019 0.015 22.8 7.4 5.2 0.64 0.22 0.15 +PG0948+632 1063572032933888256 sdB 27700 600 5.59 0.06 0.077 0.8647 0.0303 -11.158 0.005 0.027 0.179 0.007 0.006 16.9 2.4 2.3 0.45 0.08 0.07 +PG0950+120 613219762482485632 sdOB 35006 161 5.68 0.03 0.082 0.8142 0.0534 -11.282 0.017 0.006 0.142 0.010 0.009 27.2 4.2 3.6 0.35 0.06 0.05 +PG0956+359 795785941630955392 He-sdO 47988 2000 5.70 0.20 0.024 0.3864 0.0476 -11.438 0.007 0.007 0.209 0.029 0.023 208.4 74.5 52.4 0.81 0.55 0.33 +PG0957+037 3848520258923494656 sdOB 34300 800 5.45 0.08 0.266 0.4648 0.0644 -11.305 0.048 0.008 0.234 0.038 0.028 68.2 24.9 16.4 0.57 0.24 0.15 +PG1000+375 802020653597763584 sdB 31694 228 5.52 0.04 0.989 0.8106 0.0330 -10.992 0.096 0.019 0.272 0.012 0.011 66.9 6.2 5.6 0.89 0.12 0.10 +PG1000+408 803736166614876544 sdB 36400 1000 5.54 0.10 0.012 1.0203 0.0365 -11.001 0.007 0.012 0.217 0.008 0.008 74.3 10.4 9.2 0.60 0.16 0.13 +PG1009+069 3873745971947175168 sdO 58474 6000 5.62 0.20 0.035 0.4794 0.0667 -11.528 0.018 0.013 0.137 0.022 0.017 197.7 124.6 78.3 0.29 0.21 0.12 +PG1009+491 822945768622050048 sdB 28690 1039 5.54 0.16 0.074 0.2743 0.0540 -11.485 0.009 0.004 0.265 0.064 0.044 42.9 24.7 14.0 0.91 0.69 0.37 +PG1017+430 805690720332579456 sdOB 42046 519 5.32 0.04 0.010 0.3377 0.0595 -11.377 0.021 0.004 0.274 0.058 0.041 211.1 99.7 59.0 0.57 0.28 0.17 +PG1032+406 780253140863277184 sdB 31600 900 5.77 0.10 0.032 4.7305 0.0542 -10.539 0.024 0.006 0.135 0.003 0.003 16.3 2.4 2.3 0.39 0.10 0.08 +PG1033+201 3987249901607922944 sdBV 35511 103 5.73 0.03 0.484 0.5050 0.0498 -11.294 0.104 0.019 0.215 0.023 0.019 65.7 15.1 11.4 0.90 0.22 0.16 +PG1039+219 3987913113277693184 sdB 33100 900 5.64 0.10 0.017 1.9034 0.0486 -10.885 0.012 0.024 0.152 0.004 0.004 24.8 3.4 3.2 0.37 0.10 0.08 +PG1047+003 3806303066866089216 sdBV 35357 143 5.85 0.02 0.035 1.4769 0.0436 -10.982 0.006 0.030 0.158 0.005 0.005 35.0 2.6 2.5 0.64 0.05 0.05 +PG1051+501 832980633290384256 sdB 33800 900 4.96 0.10 0.047 0.7449 0.0390 -10.960 0.011 0.034 0.327 0.018 0.016 125.8 20.4 17.4 0.36 0.11 0.08 +PG1101+113 3868458111291375616 sdOB 35660 149 5.79 0.02 0.097 0.6110 0.0442 -11.302 0.012 0.013 0.181 0.014 0.012 47.4 7.8 6.3 0.74 0.13 0.10 +PG1101+249 3995631994142136576 sdB 29700 500 5.90 0.07 0.064 2.3503 0.0434 -10.728 0.046 0.051 0.177 0.004 0.004 21.8 2.2 2.1 0.91 0.16 0.14 +PG1102+499 832788184395879424 He-sdO 67647 891 5.38 0.03 0.013 0.5381 0.0458 -11.297 0.011 0.006 0.208 0.019 0.016 815.6 164.7 127.9 0.38 0.08 0.07 +PG1104+299 732692631532422528 sdB 36909 164 5.79 0.03 0.046 0.5346 0.0515 -11.422 0.007 0.005 0.157 0.017 0.014 41.2 9.4 7.1 0.56 0.13 0.10 +PG1104+476 783541848870827264 sdB 27343 456 5.72 0.06 0.138 0.5030 0.0747 -11.487 0.020 0.005 0.143 0.025 0.019 10.3 4.2 2.9 0.39 0.16 0.11 +PG1106+271 3998182792399323904 sdO 40528 2000 5.40 0.20 0.191 0.3734 0.0539 -11.374 0.035 0.010 0.247 0.041 0.031 147.5 64.8 42.2 0.57 0.41 0.24 +PG1115+201 3978207002584425216 sdB 29393 191 5.50 0.03 0.285 1.3693 0.0424 -10.791 0.016 0.048 0.263 0.009 0.008 46.4 3.5 3.3 0.80 0.08 0.07 +PG1115+275 3997846990381096192 sdO 48463 2000 5.72 0.20 0.033 0.6917 0.0683 -11.513 0.004 0.006 0.098 0.011 0.009 48.1 14.5 10.8 0.19 0.12 0.08 +PG1116+301 4023163971460301952 sdB 32500 900 5.85 0.10 0.110 1.2123 0.0398 -11.089 0.019 0.009 0.149 0.005 0.005 22.2 3.3 3.0 0.57 0.15 0.12 +PG1117+312 4023386553845346688 sdOB 33626 895 5.74 0.13 0.014 0.8632 0.0494 -11.180 0.016 0.006 0.170 0.010 0.009 33.1 5.8 5.0 0.58 0.22 0.16 +PG1118+061 3813980166288451072 sdB 28014 274 5.22 0.04 0.186 0.9275 0.0353 -11.020 0.062 0.005 0.227 0.009 0.009 28.5 2.9 2.7 0.31 0.05 0.04 +PG1119+377 760930907631979904 sdOB 37753 1052 5.53 0.14 0.016 0.3087 0.0607 -11.518 0.012 0.012 0.217 0.053 0.036 86.3 48.9 27.0 0.59 0.42 0.23 +PG1119+619 862792310530019328 sdB 29300 500 5.69 0.10 0.040 0.6202 0.0385 -11.301 0.012 0.005 0.178 0.012 0.010 21.1 3.6 3.1 0.57 0.17 0.13 +PG1125+295 4022181695259436416 sdO 70410 1499 5.51 0.04 0.015 0.6845 0.0525 -11.426 0.009 0.006 0.121 0.010 0.009 325.1 63.9 51.0 0.17 0.04 0.04 +PG1128+199 3977575573672822400 sdB 29179 1005 5.58 0.16 0.029 0.5425 0.0519 -11.336 0.026 0.006 0.187 0.020 0.016 22.9 6.3 4.9 0.49 0.25 0.17 +PG1130+054 3813295101825640704 sdB 30050 136 5.89 0.03 0.151 0.9797 0.0507 -11.130 0.009 0.008 0.168 0.009 0.009 20.8 2.7 2.5 0.80 0.11 0.10 +PG1130-063 3593223417120115712 sdO 46400 1000 5.89 0.07 0.013 0.4830 0.0698 -11.639 0.006 0.017 0.106 0.018 0.013 46.4 17.6 11.5 0.32 0.13 0.09 +PG1134+144 3918117008499710848 He-sdOB 37956 198 5.83 0.03 0.078 2.0349 0.0488 -10.941 0.008 0.010 0.125 0.004 0.004 29.3 2.1 2.0 0.39 0.04 0.04 +PG1134+463 785980977968930560 He-sdO 48889 5000 5.69 0.20 0.064 0.5247 0.0486 -11.401 0.027 0.009 0.167 0.017 0.014 143.9 77.6 53.4 0.50 0.32 0.20 +PG1135+585 846070525377462528 sdOB 35158 908 5.81 0.13 0.010 0.5330 0.0473 -11.510 0.021 0.003 0.129 0.013 0.011 22.7 5.5 4.3 0.39 0.16 0.12 +PG1136-003 3794197787442075008 sdB 31200 600 5.54 0.09 0.266 0.7979 0.0453 -11.091 0.021 0.032 0.209 0.013 0.011 37.3 5.8 4.9 0.56 0.15 0.12 +PG1138+425 769397353324856448 sdO 43313 2000 5.82 0.20 0.603 0.5470 0.0414 -11.316 0.065 0.014 0.190 0.016 0.014 114.4 31.0 24.3 0.88 0.55 0.34 +PG1140-050 3599609105776343680 sdB 34522 0 4.97 0.00 0.684 0.3032 0.0434 -11.173 0.034 0.011 0.481 0.081 0.060 295.3 107.3 68.9 0.79 0.29 0.19 +PG1142-037 3600365496761173504 sdB 30048 240 5.60 0.05 0.017 0.4166 0.0606 -11.383 0.044 0.009 0.219 0.038 0.028 35.3 13.2 8.5 0.70 0.28 0.18 +PG1151+359 4031612751951454080 sdB 29400 500 5.49 0.06 0.200 0.3104 0.0581 -11.487 0.014 0.005 0.231 0.053 0.036 35.9 18.8 10.6 0.61 0.33 0.19 +PG1153+344 4028265945931548544 sdOB 40483 275 5.54 0.03 0.039 0.5745 0.0523 -11.277 0.015 0.012 0.204 0.020 0.017 100.1 21.0 16.2 0.53 0.12 0.09 +PG1201+258 4006102059258774272 sdOB 33932 111 5.58 0.03 0.550 0.7520 0.0640 -11.177 0.139 0.026 0.186 0.017 0.015 41.1 8.1 6.3 0.48 0.10 0.08 +PG1202+404 4034847759974004992 sdB 27628 1188 5.32 0.17 0.032 0.4839 0.0481 -11.328 0.005 0.004 0.216 0.024 0.020 24.4 7.5 5.7 0.36 0.20 0.13 +PG1203+574 1575432697534110336 sdB 33620 390 5.90 0.13 0.019 0.8492 0.0353 -11.259 0.007 0.009 0.144 0.007 0.006 23.7 2.8 2.6 0.60 0.22 0.16 +PG1206+165 3922570889586104064 sdB 29584 148 5.48 0.02 0.724 1.2561 0.0438 -10.807 0.135 0.013 0.271 0.010 0.009 50.4 4.1 3.7 0.81 0.07 0.07 +PG1207-032 3598151393876907904 sdB 35693 500 5.82 0.05 0.010 2.1343 0.0483 -10.969 0.010 0.006 0.111 0.003 0.003 18.1 1.9 1.9 0.30 0.04 0.04 +PG1230+052 3708157360436901248 sdB 28300 1000 5.72 0.15 0.033 1.6131 0.0379 -10.807 0.013 0.013 0.214 0.005 0.005 26.3 4.4 3.9 0.88 0.36 0.26 +PG1233+427 1534536701840624768 sdB 26200 1100 5.31 0.12 0.046 3.0875 0.0443 -10.559 0.013 0.013 0.198 0.004 0.003 16.7 3.3 3.0 0.29 0.10 0.07 +PG1234+253 3959631234670040704 sdB 34500 1000 5.83 0.10 0.056 7.0625 0.0592 -10.356 0.006 0.009 0.138 0.002 0.002 24.4 3.3 3.1 0.47 0.12 0.10 +PG1234+505 1568451554613870848 sdO 44458 563 5.53 0.04 0.036 0.6862 0.0459 -11.281 0.021 0.011 0.169 0.012 0.011 100.0 15.9 13.0 0.35 0.07 0.06 +PG1236+479 1543006141129419648 sdB 28400 800 5.55 0.10 0.081 0.5819 0.0418 -11.314 0.016 0.008 0.185 0.014 0.013 19.9 4.3 3.6 0.44 0.14 0.11 +PG1237+132 3928807456977316992 sdB 33100 900 5.93 0.10 0.122 0.9552 0.0439 -11.190 0.007 0.011 0.152 0.008 0.007 24.8 4.1 3.6 0.72 0.20 0.16 +PG1238+515 1568569889552108800 He-sdO 43449 225 5.95 0.05 0.025 1.0853 0.0320 -11.074 0.009 0.038 0.172 0.006 0.005 95.0 6.3 5.8 0.97 0.13 0.12 +PG1239+044 3704162319296853120 sdB 34928 146 5.97 0.02 0.027 0.7185 0.0546 -11.371 0.020 0.006 0.131 0.011 0.009 23.0 4.2 3.4 0.59 0.11 0.09 +PG1239+439 1540495440685138432 sdOB 38488 264 6.00 0.05 0.076 0.3925 0.0684 -11.669 0.012 0.006 0.121 0.025 0.018 28.8 13.5 8.0 0.54 0.26 0.16 +PG1242+441 1540815913964920448 sdB 31302 259 5.63 0.07 0.631 0.5370 0.0686 -11.427 0.042 0.016 0.150 0.022 0.017 19.3 6.3 4.4 0.35 0.13 0.09 +PG1244-004 3683849391728631424 sdOB 42775 828 5.98 0.09 0.088 0.4868 0.0731 -11.606 0.020 0.005 0.112 0.020 0.015 37.9 15.0 9.7 0.44 0.21 0.13 +PG1249+761 1692116238728076544 He-sdO 37643 1143 5.73 0.06 0.106 0.4537 0.0346 -11.501 0.025 0.004 0.154 0.013 0.011 42.6 9.4 7.5 0.46 0.11 0.09 +PG1249-028 3682304199935092096 sdB 34220 300 5.91 0.06 0.062 0.5984 0.0508 -11.316 0.020 0.009 0.178 0.016 0.014 39.0 7.8 6.1 0.94 0.24 0.18 +PG1250+303 1465043619891174016 sdB 35541 211 5.98 0.04 0.011 0.5670 0.0577 -11.443 0.035 0.010 0.141 0.016 0.013 28.4 6.9 5.2 0.69 0.18 0.14 +PG1254+279 1463697233542956672 sdB 26180 267 5.57 0.03 0.071 0.5984 0.0614 -11.320 0.009 0.009 0.177 0.020 0.017 13.2 3.5 2.8 0.42 0.11 0.08 +PG1256+278 1460692714941449728 He-sdB 36625 240 5.90 0.05 0.010 1.3746 0.0544 -11.089 0.008 0.008 0.132 0.006 0.005 28.0 2.8 2.6 0.50 0.08 0.07 +PG1257+010 3689536684343245312 sdOB 40203 391 5.60 0.05 1.905 0.6569 0.0388 -11.086 0.066 0.051 0.247 0.016 0.014 143.1 19.4 16.2 0.89 0.16 0.14 +PG1258+012 3689564206493682816 He-sdOB 39359 1000 5.64 0.10 0.417 0.4421 0.0617 -11.535 0.113 0.019 0.141 0.023 0.017 43.0 15.9 10.5 0.32 0.15 0.10 +PG1300+278 1460730407575030656 sdB 29600 1000 5.65 0.15 0.062 0.8808 0.0435 -11.099 0.007 0.018 0.201 0.011 0.010 27.9 5.2 4.5 0.66 0.29 0.20 +PG1302+284 1461140216174118016 sdB 36934 113 5.91 0.02 0.011 0.7407 0.0558 -11.386 0.007 0.009 0.123 0.010 0.009 25.3 4.5 3.7 0.45 0.08 0.07 +PG1303+097 3734224925705249152 sdB 29800 500 5.83 0.05 0.064 1.1348 0.0411 -11.089 0.007 0.008 0.159 0.006 0.006 18.0 2.3 2.2 0.63 0.09 0.08 +PG1303+122 3737057611255721472 sdB 30700 200 5.45 0.03 0.037 0.4047 0.0587 -11.449 0.005 0.008 0.195 0.033 0.025 30.3 11.3 7.3 0.39 0.15 0.10 +PG1304+491 1554816510916988544 sdB 33183 112 5.76 0.02 0.013 1.4305 0.0286 -10.993 0.015 0.003 0.157 0.004 0.004 26.9 1.8 1.8 0.52 0.04 0.04 +PG1310+179 3937241226560203136 sdOB 35544 545 5.34 0.09 0.596 0.6701 0.0402 -11.213 0.075 0.014 0.197 0.013 0.011 55.7 8.3 7.0 0.31 0.09 0.07 +PG1311+372 1474359575755115136 sdB 29665 491 5.48 0.09 0.067 0.9574 0.0379 -11.108 0.012 0.006 0.180 0.008 0.007 22.7 2.9 2.6 0.36 0.09 0.07 +PG1313+132 3742799192256205056 sdB 25600 1000 5.41 0.15 0.067 1.0159 0.0437 -11.044 0.007 0.010 0.198 0.009 0.008 15.1 3.2 2.8 0.37 0.16 0.11 +PG1313+165 3744601257454417152 sdB 32371 964 5.81 0.15 0.060 0.6608 0.0468 -11.409 0.020 0.007 0.131 0.010 0.009 16.9 3.7 3.1 0.40 0.18 0.13 +PG1316+212 3940518836361346304 He-sdO 53080 372 5.63 0.06 0.027 0.4151 0.0499 -11.411 0.005 0.007 0.207 0.028 0.022 306.6 90.1 62.5 0.67 0.23 0.16 +PG1318+062 3717383603022961792 He-sdO 46503 389 5.83 0.06 0.111 0.5876 0.0461 -11.300 0.017 0.008 0.189 0.016 0.014 149.3 27.1 21.3 0.88 0.21 0.16 +PG1321+265 1449056067988016128 sdOB 36388 231 5.73 0.04 0.026 0.4170 0.0637 -11.517 0.013 0.015 0.161 0.029 0.021 41.0 16.2 10.2 0.51 0.21 0.13 +PG1322+286 1449575655951553408 sdB 32500 1710 5.82 0.36 0.074 0.6197 0.0439 -11.320 0.014 0.009 0.171 0.013 0.012 29.4 8.5 6.7 0.71 0.93 0.40 +PG1325+054 3717793239823667200 He-sdO 44492 231 5.90 0.04 0.073 0.7442 0.0442 -11.263 0.005 0.009 0.163 0.010 0.009 93.4 12.3 10.4 0.77 0.13 0.11 +PG1329+159 3744968013301724544 sdB 29100 1000 5.62 0.15 0.013 1.2605 0.0337 -10.847 0.015 0.016 0.251 0.007 0.007 40.4 6.4 5.7 0.96 0.40 0.28 +PG1336-018 3637481302758519040 sdBV 32800 500 5.76 0.05 0.031 1.7078 0.0376 -10.936 0.018 0.067 0.152 0.004 0.004 24.0 2.3 2.2 0.49 0.07 0.06 +PG1338+481 1552221800914196480 sdB 29109 205 5.46 0.03 0.062 1.2314 0.0305 -10.903 0.031 0.007 0.224 0.006 0.006 32.5 2.4 2.3 0.53 0.05 0.05 +PG1339+052 3714909426982422272 sdO 80000 2973 6.42 0.09 0.039 0.6996 0.0595 -11.630 0.033 0.008 0.073 0.007 0.006 197.9 50.8 39.4 0.52 0.16 0.12 +PG1344+114 3727881843124118400 sdB 23163 185 5.30 0.02 0.058 1.0366 0.0413 -11.111 0.024 0.008 0.166 0.007 0.007 7.1 1.5 1.5 0.20 0.03 0.03 +PG1344+285 1451833434359977216 sdB 28800 600 5.46 0.07 0.011 0.6802 0.0383 -11.158 0.006 0.009 0.227 0.014 0.012 31.8 5.0 4.3 0.54 0.12 0.10 +PG1349+659 1671349350297566976 He-sdOB 39660 867 6.14 0.13 0.068 0.6194 0.0380 -11.598 0.016 0.016 0.090 0.006 0.006 18.1 3.3 2.8 0.41 0.16 0.11 +PG1352-022 3657799934042253952 sdOB 43091 289 5.87 0.03 0.108 3.5942 0.0595 -10.762 0.018 0.014 0.107 0.003 0.003 35.4 2.1 2.0 0.31 0.03 0.03 +PG1353+152 1231024630186706944 sdB 30174 202 5.58 0.04 0.305 0.5164 0.0512 -11.330 0.122 0.017 0.194 0.021 0.017 28.1 6.7 5.0 0.52 0.14 0.10 +PG1353+162 1243253467230351360 sdOB 37330 915 5.86 0.13 0.104 0.5878 0.0644 -11.479 0.025 0.002 0.125 0.015 0.012 27.2 7.8 5.8 0.41 0.19 0.13 +PG1355+071 3720655474749294592 sdB 27680 570 5.36 0.09 0.010 0.9981 0.0439 -11.014 0.032 0.006 0.215 0.010 0.009 24.3 3.4 3.1 0.39 0.10 0.08 +PG1359+003 3660503903717853056 sdOB 33383 1218 5.90 0.13 0.157 0.4729 0.0741 -11.582 0.025 0.014 0.121 0.022 0.016 16.5 7.4 4.8 0.43 0.25 0.15 +PG1359+077 3720793562242705664 sdB 35800 300 5.48 0.09 0.851 0.6250 0.0531 -11.282 0.123 0.027 0.174 0.016 0.014 44.6 8.9 6.9 0.33 0.11 0.08 +PG1403+316 1454323415879594368 sdB 31456 108 5.73 0.02 0.028 1.7055 0.0357 -10.930 0.009 0.009 0.153 0.004 0.004 20.6 1.7 1.7 0.46 0.04 0.04 +PG1407+387 1485199008058786688 sdO 40660 576 5.09 0.05 1.096 0.4582 0.0364 -11.332 0.028 0.012 0.224 0.019 0.016 122.7 23.3 18.4 0.22 0.05 0.04 +PG1407-013 3647329074356945152 sdOB 41464 364 5.46 0.05 0.195 0.8539 0.0362 -11.023 0.014 0.017 0.246 0.011 0.010 161.1 15.7 13.8 0.64 0.10 0.09 +PG1408+098 3723006814724972416 sdB 36580 710 5.77 0.11 0.065 1.2371 0.0429 -11.106 0.010 0.023 0.141 0.005 0.005 31.8 3.8 3.4 0.43 0.13 0.10 +PG1412+299 1260997037986811648 sdB 27449 447 5.81 0.06 0.057 0.3941 0.0658 -11.462 0.043 0.004 0.194 0.038 0.028 19.2 8.6 5.4 0.89 0.42 0.26 +PG1413+114 1225417739360402048 He-sdOB 43100 800 5.81 0.17 0.058 0.3338 0.0628 -11.547 0.009 0.013 0.189 0.043 0.030 110.3 57.3 32.7 0.86 0.64 0.35 +PG1413+421 1492192692285509376 sdB 30853 214 5.67 0.04 0.127 0.9047 0.0338 -11.165 0.014 0.010 0.168 0.007 0.006 22.9 2.4 2.2 0.48 0.06 0.06 +PG1421+345 1479772643298162176 sdB 37762 641 5.19 0.08 1.778 0.6650 0.0194 -10.912 0.083 0.017 0.397 0.012 0.011 287.3 26.7 24.5 0.89 0.19 0.16 +PG1422+035 3668499109893566464 sdOB 34957 945 5.71 0.15 0.245 0.4806 0.0667 -11.527 0.040 0.008 0.136 0.022 0.017 24.7 9.2 6.3 0.35 0.20 0.12 +PG1425+019 3654573039213596672 sdB 33417 556 5.76 0.11 0.092 0.4625 0.0630 -11.425 0.011 0.011 0.180 0.028 0.022 36.3 12.6 8.5 0.69 0.32 0.21 +PG1425+219 1240669924143182592 sdB 28395 835 5.25 0.10 0.966 0.3917 0.0358 -11.169 0.045 0.013 0.373 0.037 0.031 81.3 20.2 15.5 0.91 0.31 0.23 +PG1425+590 1611954625518358272 He-sdO 43071 2324 6.00 0.34 0.014 0.4936 0.0387 -11.550 0.003 0.007 0.126 0.011 0.009 49.5 15.0 11.8 0.59 0.72 0.32 +PG1426+213 1240449403342559360 sdB 32604 140 5.52 0.03 0.202 2.2469 0.0462 -10.873 0.012 0.015 0.132 0.003 0.003 17.7 1.6 1.6 0.21 0.03 0.03 +PG1427+195 1239364769480858496 He-sdO 54412 503 5.68 0.04 0.044 0.7202 0.0408 -11.203 0.006 0.043 0.193 0.012 0.010 294.6 37.6 32.3 0.65 0.11 0.09 +PG1431+081 1172548341214173952 sdOB 36600 600 6.16 0.13 0.032 0.4914 0.0786 -11.620 0.004 0.013 0.108 0.021 0.015 19.0 8.2 5.2 0.63 0.36 0.22 +PG1432+158 1234322477875249664 sdB 29066 282 5.79 0.04 0.067 1.6038 0.0414 -10.928 0.013 0.007 0.163 0.005 0.005 17.0 1.8 1.8 0.60 0.07 0.06 +PG1432+290 1281101268798929152 sdOB 36729 915 5.94 0.13 0.507 0.4934 0.0466 -11.416 0.082 0.023 0.165 0.017 0.014 44.5 10.9 8.4 0.87 0.37 0.26 +PG1437+233 1242599704488616704 sdB 29904 185 5.43 0.03 0.140 0.6829 0.0355 -11.155 0.017 0.009 0.225 0.013 0.011 36.4 4.4 3.8 0.50 0.07 0.06 +PG1438+018 3655309299687364992 sdB 30687 291 5.87 0.06 0.339 1.1558 0.0402 -10.995 0.025 0.012 0.189 0.007 0.007 28.5 2.7 2.6 0.97 0.16 0.14 +PG1438+056 1159067504023867904 sdB 31763 1433 5.69 0.15 0.127 0.4644 0.0591 -11.510 0.006 0.008 0.149 0.022 0.017 20.3 7.8 5.5 0.40 0.22 0.14 +PG1438-029 3648191164488514688 sdB 32255 162 5.76 0.03 0.316 1.2947 0.0362 -10.925 0.017 0.007 0.203 0.006 0.006 40.0 2.8 2.7 0.86 0.08 0.08 +PG1439-013 3649025693813906304 sdO 40045 602 5.70 0.08 0.083 0.8309 0.0373 -11.072 0.004 0.040 0.227 0.011 0.010 118.7 13.8 12.0 0.94 0.21 0.18 +PG1444+076 1171708967165771392 He-sdO 52839 402 5.91 0.02 0.025 0.5981 0.0498 -11.315 0.006 0.007 0.180 0.016 0.014 226.2 43.4 33.8 0.96 0.19 0.15 +PG1451+397 1296418427846820608 sdB 32680 239 5.89 0.05 0.047 0.5978 0.0459 -11.449 0.015 0.004 0.132 0.011 0.010 17.7 3.4 2.8 0.49 0.11 0.09 +PG1452+198 1237226700401153792 sdB 31177 70 5.82 0.02 0.023 2.9859 0.0466 -10.711 0.013 0.021 0.145 0.003 0.003 17.8 1.5 1.5 0.51 0.04 0.04 +PG1452+475 1590388529573233536 sdB 27233 1102 5.57 0.16 0.082 0.4422 0.0432 -11.439 0.006 0.004 0.183 0.020 0.016 16.5 5.1 3.9 0.46 0.24 0.16 +PG1454+502 1592429562456407424 sdB 30810 1050 5.58 0.16 0.257 0.2702 0.0466 -11.522 0.037 0.007 0.244 0.050 0.036 48.1 23.4 14.1 0.84 0.58 0.33 +PG1455+501 1592412936639159424 sdOB 33401 1028 5.16 0.16 1.175 0.5376 0.0263 -11.093 0.040 0.016 0.322 0.017 0.015 116.4 19.7 16.8 0.55 0.25 0.17 +PG1457+193 1188933362275187200 sdOB 37350 1090 5.92 0.15 0.176 1.3201 0.0360 -11.128 0.012 0.014 0.125 0.004 0.004 27.4 4.0 3.6 0.48 0.20 0.14 +PG1458+423 1585277243613047936 sdB 30265 147 5.39 0.03 0.031 1.1271 0.0304 -11.002 0.017 0.005 0.196 0.006 0.005 28.8 2.2 2.1 0.34 0.04 0.04 +PG1501+426 1393235511913580800 sdB 29170 380 5.52 0.12 0.080 0.9394 0.0283 -11.130 0.006 0.004 0.175 0.006 0.005 19.9 2.2 2.1 0.37 0.12 0.09 +PG1502+113 1180527806334711936 sdB 33200 500 5.80 0.10 0.088 0.7998 0.0504 -11.332 0.007 0.010 0.129 0.009 0.008 18.2 3.1 2.7 0.39 0.12 0.09 +PG1507-015 4418117477394214400 He-sdO 49800 936 6.12 0.12 0.398 0.4254 0.0679 -11.567 0.032 0.015 0.141 0.027 0.019 110.1 46.6 29.0 0.97 0.53 0.32 +PG1508+177 1211503282272546432 sdB 31951 290 5.37 0.05 1.135 0.4499 0.0449 -11.243 0.099 0.016 0.273 0.030 0.025 69.9 16.6 12.3 0.64 0.17 0.13 +PG1512+244 1264108144792924160 sdB 29900 900 5.74 0.10 0.116 2.1904 0.0329 -10.865 0.022 0.015 0.139 0.003 0.003 13.8 2.3 2.2 0.39 0.10 0.08 +PG1518+299 1275262415380252544 sdOB 41746 293 5.98 0.04 0.079 0.6702 0.0505 -11.455 0.025 0.010 0.116 0.010 0.008 36.6 6.4 5.2 0.47 0.10 0.08 +PG1521+357 1375081784665146496 sdOB 37656 2000 5.64 0.20 0.188 0.3774 0.0480 -11.576 0.039 0.007 0.155 0.022 0.018 43.4 17.5 12.1 0.39 0.27 0.16 +PG1522+306 1276808981563720576 sdO 51880 1839 5.30 0.07 1.096 0.3629 0.0343 -11.314 0.050 0.024 0.282 0.029 0.024 515.8 140.9 105.5 0.58 0.17 0.13 +PG1522-013 4415381450083363968 sdB 25922 908 5.31 0.10 0.398 0.8244 0.0327 -11.077 0.020 0.010 0.224 0.009 0.009 20.4 3.8 3.4 0.37 0.11 0.08 +PG1525+024 4420981434602491520 sdB 27133 1277 5.14 0.18 0.295 0.6592 0.0376 -11.270 0.006 0.011 0.181 0.011 0.010 15.9 4.1 3.5 0.17 0.09 0.06 +PG1525+107 1165848673269627520 sdOB 36438 198 5.86 0.04 0.153 0.5213 0.0668 -11.459 0.002 0.018 0.148 0.022 0.017 34.8 11.0 7.6 0.58 0.19 0.13 +PG1528+029 4421118770476595200 He-sdO 45548 2000 5.72 0.20 0.136 0.4626 0.0445 -11.443 0.007 0.008 0.173 0.018 0.015 116.3 35.1 26.3 0.58 0.37 0.23 +PG1528+062 4429114659552190080 sdOB 34443 103 5.99 0.02 0.124 1.2313 0.0412 -11.197 0.022 0.007 0.114 0.004 0.004 16.5 1.8 1.8 0.47 0.05 0.04 +PG1528+104 1165963744033018496 sdB 28954 271 5.69 0.04 0.087 1.4799 0.0317 -10.845 0.010 0.011 0.214 0.005 0.005 28.9 2.2 2.1 0.82 0.09 0.08 +PG1530+431 1391344214475144832 sdB 35911 408 5.31 0.05 1.216 0.5718 0.0280 -11.099 0.032 0.021 0.295 0.015 0.014 129.9 15.2 13.1 0.65 0.11 0.09 +PG1531+447 1394581623383963264 sdB 30963 155 5.69 0.03 0.063 0.7233 0.0361 -11.314 0.012 0.009 0.149 0.008 0.007 18.3 2.4 2.2 0.40 0.06 0.05 +PG1538+269 1223920926079402112 sdB 26841 352 5.49 0.04 0.120 1.2256 0.0297 -10.909 0.008 0.011 0.224 0.006 0.006 23.3 2.2 2.1 0.56 0.07 0.06 +PG1538+401 1377891689708857856 sdB 36741 161 5.76 0.03 0.021 2.4233 0.0305 -10.914 0.009 0.005 0.111 0.002 0.002 20.3 1.5 1.5 0.26 0.03 0.03 +PG1544+253 1222767813259931776 He-sdO 55000 3000 5.60 0.50 0.075 0.7354 0.0380 -11.184 0.026 0.017 0.197 0.011 0.010 320.3 85.8 69.0 0.56 1.22 0.38 +PG1544+277 1224427182464055680 sdB 34269 245 5.55 0.05 0.110 0.3085 0.0489 -11.550 0.015 0.010 0.203 0.038 0.028 50.9 21.1 13.1 0.53 0.23 0.15 +PG1544+488 1401621384019650560 He-sdB 38444 152 5.77 0.04 0.076 2.0142 0.0354 -10.860 0.007 0.010 0.153 0.003 0.003 46.0 2.3 2.2 0.50 0.06 0.05 +PG1546+045 4426202946603971968 sdB 33384 224 6.05 0.05 0.355 0.8564 0.0435 -11.292 0.010 0.009 0.132 0.007 0.007 19.4 2.6 2.4 0.71 0.12 0.10 +PG1548+166 1196375273586921472 sdB 33223 107 5.78 0.02 0.090 0.6879 0.0427 -11.204 0.015 0.008 0.201 0.013 0.012 44.1 6.2 5.2 0.89 0.13 0.11 +PG1549+006 4410613624072340736 sdB 37227 465 5.80 0.07 0.343 0.7612 0.0386 -11.254 0.036 0.009 0.160 0.009 0.008 44.1 5.6 4.8 0.59 0.13 0.10 +PG1549-001 4410368536057777024 sdB 28252 500 5.49 0.05 0.269 0.6882 0.0414 -11.178 0.006 0.006 0.214 0.014 0.012 26.3 4.2 3.6 0.52 0.10 0.08 +PG1553+272 1220472582737099776 sdB 22100 900 4.74 0.10 0.148 0.7864 0.0256 -10.794 0.012 0.010 0.454 0.015 0.014 44.1 8.4 7.3 0.41 0.11 0.09 +PG1554+222 1206214356465503616 He-sdO 66508 938 5.34 0.04 0.160 0.6649 0.0320 -11.160 0.020 0.007 0.230 0.012 0.011 928.4 110.9 96.7 0.42 0.06 0.06 +PG1554+408 1383048811559130240 He-sdB 37700 200 5.20 0.10 0.031 0.2685 0.0489 -11.589 0.045 0.009 0.213 0.047 0.033 82.4 40.4 23.4 0.26 0.16 0.09 +PG1555+504 1403149533383468928 He-sdO 71231 7000 5.84 0.20 0.013 0.3302 0.0422 -11.651 0.004 0.006 0.150 0.022 0.017 524.4 307.4 197.7 0.58 0.40 0.24 +PG1559+048 4425487989169416320 He-sdOB 40511 312 5.76 0.07 0.151 1.4154 0.0431 -11.184 0.013 0.019 0.103 0.004 0.004 25.5 2.3 2.2 0.22 0.05 0.04 +PG1559+533 1404827731724827776 sdB 31119 164 5.67 0.03 0.038 1.3414 0.0260 -11.083 0.005 0.004 0.136 0.003 0.003 15.7 1.6 1.6 0.32 0.03 0.03 +PG1605+072 4450489165598124800 sdBV 32576 333 5.23 0.05 0.123 1.3807 0.0597 -10.800 0.012 0.020 0.255 0.012 0.011 66.0 6.8 6.0 0.40 0.07 0.06 +PG1606+388 1379038445977180928 sdOB 34684 968 5.78 0.18 0.070 0.4030 0.0472 -11.657 0.046 0.006 0.121 0.016 0.013 19.0 6.1 4.4 0.32 0.20 0.12 +PG1607+227 1206447693448896128 He-sdO 45362 2000 5.86 0.20 0.302 0.3200 0.0565 -11.584 0.008 0.011 0.181 0.038 0.027 124.3 65.5 38.6 0.88 0.71 0.38 +PG1609+195 1201659389029469184 sdOB 33136 918 5.73 0.13 0.017 0.5588 0.0471 -11.423 0.013 0.010 0.150 0.014 0.012 24.2 5.7 4.6 0.44 0.18 0.13 +PG1610+043 4437254653372798848 He-sdO 45059 2000 5.81 0.20 0.219 0.3919 0.0539 -11.542 0.010 0.022 0.162 0.026 0.020 97.6 39.6 26.4 0.62 0.45 0.26 +PG1610+519 1427678435208512384 sdOB 48506 629 5.24 0.08 0.385 0.9510 0.0370 -10.973 0.082 0.010 0.246 0.010 0.009 300.3 29.5 26.5 0.38 0.09 0.07 +PG1610+529 1427969118595251072 sdB 31112 182 5.71 0.04 0.099 2.3455 0.0361 -10.771 0.006 0.014 0.160 0.003 0.003 21.6 1.6 1.6 0.48 0.05 0.05 +PG1611+041 4437211291383115392 He-sdO 46096 394 5.70 0.06 0.188 0.3732 0.0451 -11.456 0.016 0.007 0.208 0.028 0.022 175.8 51.7 35.9 0.80 0.27 0.19 +PG1611+090 4452964853466754048 sdB 31840 310 5.87 0.09 0.124 1.0963 0.0381 -11.159 0.014 0.007 0.140 0.005 0.005 18.1 2.1 2.0 0.53 0.13 0.11 +PG1613+426 1381954385173920640 sdBV 35487 177 6.05 0.04 0.035 1.0083 0.0305 -11.160 0.009 0.009 0.152 0.005 0.005 33.0 2.6 2.5 0.95 0.11 0.10 +PG1616+144 4463625890008114944 sdB 36500 900 6.02 0.10 0.209 1.8174 0.0331 -10.954 0.013 0.014 0.136 0.003 0.003 29.3 3.5 3.3 0.70 0.19 0.15 +PG1617+309 1319053146015474688 sdOB 38199 274 5.92 0.04 0.091 0.7394 0.0380 -11.417 0.014 0.012 0.115 0.006 0.006 25.1 3.2 2.9 0.40 0.06 0.06 +PG1621+476 1410860511508492288 sdB 29000 600 5.65 0.06 0.050 0.5469 0.0445 -11.429 0.019 0.008 0.149 0.013 0.011 14.1 3.2 2.7 0.36 0.09 0.07 +PG1622+411 1380974582874497280 sdB 27590 430 5.29 0.06 0.302 0.7330 0.0328 -11.036 0.066 0.007 0.275 0.013 0.012 39.4 4.8 4.3 0.54 0.10 0.08 +PG1623+386 1332156747638095488 sdOB 46844 1289 5.83 0.11 0.398 0.4659 0.0383 -11.370 0.048 0.012 0.200 0.018 0.015 173.8 38.9 30.4 1.00 0.35 0.26 +PG1624+382 1332004327838630272 He-sdO 47414 2000 5.85 0.20 0.048 0.4784 0.0432 -11.505 0.005 0.006 0.145 0.014 0.012 95.2 26.9 20.5 0.55 0.35 0.21 +PG1627+006 4431621992740777088 sdB 24696 698 5.28 0.08 0.186 0.9281 0.0401 -11.062 0.039 0.006 0.206 0.010 0.009 14.2 2.6 2.4 0.30 0.07 0.06 +PG1627+112 4458994472154612480 sdB 26973 326 5.08 0.04 0.240 1.2519 0.0731 -11.011 0.014 0.024 0.173 0.011 0.010 14.3 2.4 2.2 0.13 0.03 0.03 +PG1629+081 4440145853560129408 sdOB 38110 680 5.38 0.09 0.158 1.1669 0.0392 -10.856 0.186 0.011 0.263 0.009 0.009 130.8 13.6 12.1 0.61 0.15 0.12 +PG1629+179 4467169787783133312 sdB 38701 361 5.84 0.05 0.104 0.5756 0.0575 -11.476 0.010 0.008 0.129 0.014 0.012 33.3 8.0 6.0 0.42 0.11 0.09 +PG1634+061 4435849168273656704 sdB 31278 112 5.88 0.03 0.157 2.0485 0.0859 -10.968 0.008 0.017 0.117 0.005 0.005 11.7 1.8 1.7 0.38 0.05 0.04 +PG1641+331 1314330017723952000 sdB 27900 500 5.62 0.07 0.040 0.3793 0.0460 -11.471 0.005 0.009 0.197 0.027 0.021 21.2 6.6 4.7 0.59 0.21 0.15 +PG1644+403 1355775219474985856 sdB 31082 278 5.85 0.07 0.014 1.2857 0.0280 -10.999 0.011 0.005 0.172 0.004 0.004 24.9 2.0 1.9 0.77 0.14 0.12 +PG1646+250 1300121926607765760 sdB 22001 1143 5.58 0.16 0.376 0.9095 0.0377 -11.261 0.013 0.008 0.133 0.006 0.006 3.8 1.7 1.6 0.25 0.11 0.08 +PG1646+354 1327036803023683712 sdB 27520 856 5.64 0.11 0.082 0.3934 0.0447 -11.479 0.021 0.004 0.186 0.024 0.019 17.9 5.7 4.2 0.56 0.23 0.16 +PG1648+536 1425987175870116864 sdB 33698 148 5.75 0.03 0.216 1.1785 0.0248 -11.014 0.014 0.009 0.182 0.004 0.004 38.2 2.3 2.2 0.68 0.06 0.06 +PG1652+159 4557895027682278784 He-sdOB 44326 263 5.76 0.06 0.234 0.5182 0.0393 -11.365 0.005 0.010 0.185 0.015 0.013 118.5 20.5 16.3 0.72 0.17 0.13 +PG1652+307 1312842039189917952 sdB 24900 800 5.64 0.05 0.079 0.6490 0.0352 -11.255 0.007 0.025 0.191 0.011 0.010 12.6 2.7 2.4 0.58 0.10 0.09 +PG1653+115 4447960529371137664 sdOB 36739 2000 5.23 0.20 0.724 0.5282 0.0436 -11.117 0.045 0.014 0.310 0.028 0.024 158.0 49.1 38.0 0.60 0.38 0.23 +PG1653+131 4449162845336419840 sdB 25600 900 5.40 0.10 0.035 0.9544 0.0347 -11.044 0.015 0.018 0.210 0.008 0.008 17.0 3.2 2.9 0.40 0.11 0.09 +PG1700+198 4561230774157695232 He-sdO 44300 600 5.79 0.11 0.234 0.4514 0.0383 -11.470 0.013 0.011 0.167 0.016 0.013 96.0 19.4 15.0 0.63 0.22 0.16 +PG1700+486 1408382624616093312 sdB 26010 1110 5.18 0.09 0.073 0.8078 0.0245 -11.000 0.015 0.031 0.275 0.009 0.008 31.1 6.2 5.4 0.42 0.10 0.08 +PG1703+355 1338485777087459072 He-sdO 44552 182 5.94 0.05 0.016 0.4616 0.0326 -11.479 0.007 0.007 0.159 0.012 0.011 90.0 14.3 11.7 0.81 0.16 0.13 +PG1707+214 4567834303554972288 sdOB 36795 203 5.91 0.03 0.136 0.6506 0.0397 -11.394 0.009 0.013 0.138 0.009 0.008 31.4 4.5 3.8 0.57 0.09 0.08 +PG1710+490 1414187320160273024 sdB 30600 500 5.66 0.05 0.052 2.1667 0.0317 -10.772 0.009 0.007 0.173 0.003 0.003 23.6 2.2 2.2 0.50 0.07 0.06 +PG1715+273 4574334135261377152 He-sdOB 40815 107 6.03 0.03 0.176 0.3594 0.0533 -11.671 0.003 0.011 0.131 0.023 0.017 42.8 16.1 10.4 0.67 0.26 0.17 +PG1717+474 1365071418489267584 sdOB 46643 809 6.16 0.06 0.090 0.6549 0.0385 -11.466 0.042 0.006 0.115 0.007 0.007 56.6 8.5 7.2 0.70 0.14 0.12 +PG1722+286 4598511330803479936 sdB 35800 900 5.94 0.10 0.029 2.0895 0.0272 -10.972 0.012 0.048 0.113 0.002 0.002 18.9 2.5 2.3 0.41 0.11 0.09 +PG1724+278 4598203433188549120 sdB 32600 500 5.84 0.05 0.112 0.6186 0.0400 -11.453 0.032 0.003 0.126 0.009 0.008 16.1 2.9 2.5 0.40 0.08 0.07 +PG1725+252 4570629777508086400 sdB 28900 900 5.54 0.10 0.048 1.7139 0.0305 -10.767 0.014 0.012 0.222 0.004 0.004 30.9 4.4 4.0 0.62 0.17 0.13 +PG1725+373 1337242538672314112 sdOB 33981 182 5.81 0.05 0.638 0.7139 0.0297 -11.252 0.094 0.019 0.167 0.007 0.007 33.3 3.4 3.0 0.66 0.10 0.09 +PG1733+326 4601722763749694592 sdOB 31350 926 5.76 0.13 0.130 0.8568 0.0328 -11.242 0.013 0.009 0.148 0.006 0.006 19.1 3.2 2.9 0.46 0.17 0.12 +PG1739+489 1363886900869046656 sdB 27998 264 5.45 0.03 0.061 1.5614 0.0303 -10.818 0.013 0.005 0.215 0.005 0.005 25.5 2.0 1.9 0.47 0.04 0.04 +PG1743+477 1362888819188840320 sdB 25500 900 5.41 0.10 0.033 1.3006 0.0242 -10.920 0.011 0.006 0.205 0.004 0.004 16.0 2.8 2.6 0.39 0.11 0.08 +PG2059+013 1729653290822954880 sdB 35380 110 5.80 0.02 0.219 0.8823 0.0448 -11.237 0.011 0.021 0.146 0.008 0.007 29.9 3.6 3.2 0.49 0.06 0.06 +PG2110+001 2689621671669850368 He-sdO 45381 2000 5.82 0.20 0.351 0.3492 0.0659 -11.582 0.008 0.008 0.168 0.039 0.027 107.2 60.7 34.7 0.69 0.58 0.31 +PG2115+145 1759463868550744576 sdB 28306 201 5.42 0.03 0.209 0.9129 0.0417 -11.173 0.020 0.008 0.163 0.008 0.007 15.3 2.1 2.0 0.26 0.04 0.04 +PG2122+157 1783691847786812288 sdB 26015 0 5.22 0.00 1.230 0.8593 0.0355 -10.836 0.096 0.019 0.363 0.016 0.015 54.3 5.0 4.5 0.80 0.07 0.07 +PG2124+071 1739298997095482240 sdB 37334 487 5.20 0.06 1.660 1.0025 0.0211 -10.787 0.057 0.011 0.354 0.008 0.008 218.8 15.1 14.2 0.73 0.11 0.10 +PG2128+112 1745849337621677184 sdOB 37868 933 6.02 0.13 0.207 0.7022 0.0469 -11.462 0.008 0.010 0.109 0.008 0.007 22.1 4.3 3.6 0.46 0.18 0.13 +PG2131+164 1772138591918813056 sdOB 39741 272 5.55 0.03 0.209 0.9543 0.0354 -11.159 0.012 0.013 0.161 0.006 0.006 58.2 5.1 4.6 0.34 0.04 0.04 +PG2132+095 1741581170917641728 sdB 37034 120 5.93 0.02 0.085 0.6804 0.0505 -11.398 0.043 0.008 0.130 0.011 0.009 28.6 5.0 4.1 0.53 0.09 0.08 +PG2201+145 1768493259900525312 He-sdO 44294 217 5.90 0.04 0.180 0.6114 0.0484 -11.492 0.006 0.007 0.116 0.010 0.009 46.6 8.5 6.8 0.39 0.08 0.07 +PG2204+034 2684009283284602880 sdB 33909 146 6.13 0.04 0.069 1.6100 0.0413 -11.085 0.008 0.009 0.113 0.004 0.003 15.3 1.6 1.6 0.63 0.07 0.07 +PG2205+023 2683585696429935488 sdB 27100 500 5.51 0.05 0.200 1.4296 0.0339 -10.977 0.013 0.011 0.164 0.004 0.004 13.0 1.8 1.8 0.32 0.05 0.04 +PG2208+014 2682170350087374464 sdB 24277 500 5.67 0.05 0.080 1.0250 0.0666 -11.277 0.008 0.017 0.114 0.008 0.007 4.1 1.6 1.5 0.22 0.05 0.04 +PG2215+120 2727702466623387648 sdOB 40100 500 5.60 0.05 0.275 0.3616 0.0626 -11.736 0.006 0.010 0.113 0.023 0.017 29.5 13.7 8.2 0.18 0.09 0.06 +PG2218+051 2708400230759920768 He-sdOB 36593 233 5.66 0.04 0.202 1.0323 0.0428 -11.305 0.006 0.009 0.106 0.005 0.005 18.2 2.2 2.0 0.19 0.03 0.03 +PG2220+006 2679230771390593024 sdO 52261 5000 5.32 0.20 0.257 0.3172 0.0611 -11.587 0.012 0.012 0.181 0.043 0.029 221.7 165.0 91.4 0.26 0.22 0.12 +PG2223+143 2732982626402453888 sdB 35020 820 5.26 0.15 0.202 0.8875 0.0764 -11.022 0.007 0.016 0.237 0.022 0.019 76.3 16.9 13.3 0.38 0.18 0.12 +PG2228+120 2730881326537936896 sdOB 44139 370 5.79 0.04 0.170 0.4468 0.0646 -11.432 0.006 0.005 0.183 0.031 0.023 114.7 42.4 27.5 0.76 0.29 0.19 +PG2236+134 2731836527264665856 sdB 31566 995 5.48 0.14 0.138 0.6809 0.0479 -11.210 0.006 0.004 0.201 0.015 0.013 36.0 7.7 6.2 0.45 0.19 0.13 +PG2237+018 2654860474117747200 sdB 25606 500 5.38 0.05 0.380 0.5728 0.0530 -11.314 0.008 0.016 0.188 0.019 0.016 13.7 3.4 2.8 0.31 0.08 0.06 +PG2240+105 2717582699040219392 sdOB 35278 130 5.73 0.03 0.148 0.8315 0.0438 -11.265 0.003 0.008 0.145 0.008 0.007 29.3 3.7 3.2 0.41 0.06 0.05 +PG2244+152 2732552133240294272 He-sdO 42144 173 5.74 0.04 0.232 0.5794 0.0530 -11.450 0.008 0.027 0.136 0.014 0.012 52.6 11.3 8.6 0.37 0.09 0.07 +PG2254+067 2712047826225618048 sdB 28500 500 5.64 0.05 0.260 0.9308 0.0492 -11.223 0.007 0.013 0.144 0.008 0.007 12.2 2.2 2.0 0.33 0.06 0.05 +PG2259+134 2815153223450428032 sdB 31078 96 5.61 0.02 0.484 1.1934 0.0467 -11.042 0.018 0.014 0.175 0.007 0.007 25.7 2.6 2.4 0.46 0.05 0.04 +PG2314+076 2665713164985202816 sdB 27200 500 5.65 0.05 0.316 2.0317 0.0379 -10.914 0.010 0.046 0.133 0.003 0.003 8.7 1.6 1.6 0.29 0.04 0.04 +PG2317+046 2660835289023309696 sdOB 40600 500 5.96 0.10 0.385 2.2897 0.0505 -10.825 0.142 0.043 0.144 0.004 0.004 50.6 3.7 3.5 0.69 0.18 0.15 +PG2323+049 2661097763064489600 sdB 28799 256 5.31 0.03 0.251 0.7104 0.0537 -11.241 0.009 0.016 0.179 0.015 0.013 19.8 3.7 3.1 0.24 0.05 0.04 +PG2331+038 2659982617755889152 sdB 27286 780 5.67 0.10 0.200 0.9722 0.0357 -11.062 0.004 0.010 0.198 0.008 0.007 19.5 3.1 2.9 0.67 0.18 0.14 +PG2331+075 2757798676856242432 sdB 31201 1115 6.19 0.12 0.389 0.9230 0.0720 -11.398 0.018 0.010 0.096 0.008 0.007 7.9 2.3 2.1 0.52 0.20 0.14 +PG2337+070 2757157489778320000 sdB 30361 152 5.61 0.03 0.582 2.2099 0.0323 -10.814 0.011 0.013 0.157 0.003 0.003 18.7 1.6 1.6 0.36 0.04 0.03 +PG2346+149 2771509999172112896 sdB 29141 1073 5.45 0.16 0.562 0.5169 0.0978 -11.258 0.060 0.015 0.230 0.053 0.037 34.3 19.0 10.9 0.55 0.41 0.22 +PG2355+242 2851511427281425536 sdOB 58136 1454 5.74 0.07 0.432 0.4082 0.0662 -11.581 0.003 0.013 0.143 0.028 0.020 208.7 92.3 56.8 0.41 0.19 0.12 +PG2358+107 2765454164004531328 sdB 27939 216 5.49 0.03 0.157 1.6454 0.0352 -10.859 0.006 0.009 0.186 0.005 0.004 19.0 1.7 1.7 0.39 0.04 0.04 +PG2359+197 2846319155418023424 sdB 31434 500 5.56 0.05 0.148 0.4198 0.0496 -11.349 0.010 0.018 0.237 0.031 0.025 49.5 14.5 10.3 0.75 0.23 0.17 +PHL48 2667642399870553984 sdB 26124 370 5.71 0.05 0.200 1.4836 0.0425 -10.828 0.013 0.044 0.222 0.007 0.006 20.6 2.2 2.1 0.92 0.13 0.11 +PN-K2-2 3158419684195782656 sdO 65883 520 6.02 0.02 0.098 1.2297 0.0471 -11.277 0.011 0.009 0.095 0.004 0.004 152.1 13.3 12.0 0.34 0.04 0.04 +PTF1J082340.04+081936.5 599294211494840704 sdB 27100 500 5.50 0.05 0.025 0.8072 0.0448 -11.133 0.004 0.013 0.203 0.012 0.011 19.9 3.2 2.8 0.47 0.08 0.07 +RWT105 252329740960393984 sdB 26250 272 5.40 0.03 0.832 2.4236 0.0792 -10.917 0.007 0.009 0.110 0.004 0.004 5.2 1.5 1.5 0.11 0.02 0.02 +RWT114 201146826149598464 sdB 32443 295 5.52 0.06 0.617 0.8771 0.0386 -11.239 0.010 0.007 0.146 0.007 0.006 21.2 2.6 2.4 0.26 0.05 0.04 +SBSS1709+535 1419133610657016064 sdB 26315 259 5.60 0.03 0.012 2.8516 0.0345 -10.657 0.026 0.005 0.171 0.003 0.003 12.6 1.5 1.5 0.42 0.04 0.04 +SDSSJ002323.99-002953.3 2542201695238975232 sdB 29200 500 5.69 0.05 0.140 0.6062 0.0533 -11.314 0.013 0.012 0.178 0.017 0.014 20.7 4.7 3.7 0.57 0.14 0.11 +SDSSJ002852.25+135446.5 2779906694594683264 sdOB 38830 1000 5.38 0.10 0.197 0.3865 0.0540 -11.480 0.014 0.010 0.190 0.031 0.023 74.1 27.4 18.2 0.32 0.14 0.10 +SDSSJ005147.75+270013.5 2808769596378258048 sdB 33163 150 5.91 0.06 0.090 0.8895 0.0622 -11.389 0.046 0.007 0.102 0.008 0.007 11.3 2.3 2.0 0.31 0.07 0.06 +SDSSJ010617.80+413434.0 374540943716955392 sdB 28089 223 5.35 0.03 0.335 0.4414 0.0471 -11.292 0.039 0.013 0.256 0.030 0.025 36.7 9.4 6.9 0.54 0.14 0.11 +SDSSJ011857.20-002546.5 2533806305483837440 sdB 27900 600 5.55 0.07 0.462 0.6610 0.0542 -11.085 0.043 0.018 0.273 0.024 0.021 40.4 8.6 6.8 0.96 0.25 0.20 +SDSSJ012340.69+300232.16 309391787394140288 sdB 31386 257 5.56 0.06 0.708 0.3890 0.0692 -11.360 0.027 0.012 0.250 0.054 0.037 54.3 26.0 15.2 0.83 0.42 0.25 +SDSSJ012739.35+404357.8 324100121943178240 sdO 48300 3200 5.67 0.10 0.060 0.4480 0.0891 -11.747 0.015 0.007 0.088 0.022 0.015 38.4 25.4 14.1 0.13 0.09 0.05 +SDSSJ013417.81+262319.2 295620885292213248 sdB 30000 198 5.60 0.04 0.335 0.3793 0.0640 -11.368 0.039 0.008 0.250 0.051 0.036 45.5 20.4 12.2 0.91 0.42 0.25 +SDSSJ021617.10-095513.0 5152094368572046336 sdOB 37001 905 5.98 0.13 0.040 0.6167 0.0554 -11.461 0.008 0.005 0.124 0.012 0.010 26.0 6.2 4.9 0.54 0.23 0.16 +SDSSJ030211.57+371109.5 142086971376178688 sdO 39468 2000 6.08 0.20 0.272 0.7521 0.0472 -11.352 0.017 0.009 0.131 0.009 0.008 37.6 10.0 8.1 0.76 0.46 0.29 +SDSSJ030859.88+380104.2 139566718927185408 sdOB 30842 963 5.68 0.14 0.543 0.4769 0.0555 -11.407 0.009 0.009 0.182 0.024 0.019 26.8 8.6 6.2 0.58 0.29 0.19 +SDSSJ031234.62+412038.6 239183090879100160 sdOB 34251 928 5.66 0.14 0.229 0.4513 0.0734 -11.586 0.006 0.011 0.128 0.025 0.018 20.2 9.0 5.7 0.28 0.17 0.10 +SDSSJ031823.06+415521.7 239492156726524544 sdOB 33841 904 5.72 0.13 0.933 0.9068 0.0555 -11.054 0.063 0.019 0.208 0.014 0.012 51.2 9.2 7.6 0.83 0.32 0.23 +SDSSJ031858.70+435539.7 242105008671742976 sdB 28572 170 5.76 0.03 0.646 0.8422 0.0696 -11.370 0.009 0.008 0.112 0.010 0.009 7.5 2.0 1.8 0.26 0.06 0.05 +SDSSJ032101.29+185719.0 56252977678408192 sdB 30205 230 5.84 0.05 0.495 0.5297 0.0649 -11.357 0.036 0.008 0.182 0.026 0.020 24.7 7.6 5.3 0.84 0.28 0.19 +SDSSJ034638.36-054359.6 3244525673877070976 sdOB 34093 901 5.98 0.13 0.282 1.2081 0.0438 -11.204 0.012 0.009 0.115 0.005 0.004 15.9 2.6 2.4 0.46 0.17 0.12 +SDSSJ034822.29+113303.4 36876009385300352 He-sdO 43804 2000 5.84 0.20 0.861 0.4736 0.0575 -11.469 0.007 0.008 0.159 0.022 0.017 83.8 30.4 21.6 0.65 0.44 0.26 +SDSSJ041149.04+152259.1 3311822554365339776 sdOB 37327 163 5.75 0.02 1.072 1.3089 0.0319 -11.033 0.008 0.023 0.158 0.004 0.004 43.4 2.7 2.6 0.51 0.04 0.04 +SDSSJ041700.67+350717.2 176164272695455744 He-sdOB 44105 352 6.03 0.08 0.881 0.5948 0.0917 -11.595 0.012 0.017 0.095 0.017 0.013 30.4 12.1 7.7 0.35 0.16 0.10 +SDSSJ044715.48+203958.2 3411847601045302144 sdB 31862 202 5.86 0.05 1.084 1.2530 0.0390 -11.124 0.006 0.020 0.134 0.005 0.004 16.6 1.8 1.8 0.47 0.07 0.06 +SDSSJ045219.32+215207.0 3412036236008926464 He-sdOB 51318 1103 6.42 0.08 0.785 0.6342 0.0559 -11.541 0.020 0.015 0.100 0.010 0.008 62.7 14.1 10.9 0.97 0.28 0.22 +SDSSJ052300.57+182727.0 3400623129219934336 He-sdB 40336 113 5.72 0.02 0.851 0.6507 0.0700 -11.478 0.006 0.028 0.114 0.014 0.011 30.7 8.0 5.9 0.25 0.07 0.05 +SDSSJ053205.85+631317.2 287317953300908672 sdB 28950 1267 5.00 0.20 0.550 0.4704 0.0427 -11.374 0.012 0.009 0.200 0.020 0.017 25.2 7.5 5.7 0.15 0.10 0.06 +SDSSJ055808.88+822218.6 557301216730452864 sdOB 35684 930 5.81 0.14 0.299 0.6065 0.0398 -11.414 0.017 0.012 0.140 0.010 0.009 28.7 5.5 4.6 0.47 0.19 0.14 +SDSSJ060715.72+643007.6 1008543468830111744 sdOB 35641 1128 5.17 0.16 1.084 0.2690 0.0432 -11.320 0.059 0.011 0.386 0.074 0.053 217.0 97.1 60.3 0.82 0.54 0.31 +SDSSJ061313.04+345600.6 3452480293768439296 sdB 29420 202 5.43 0.04 0.596 1.1253 0.0253 -10.983 0.007 0.018 0.205 0.005 0.005 28.3 2.1 2.0 0.41 0.05 0.05 +SDSSJ061401.59+332927.6 3440046359151100032 sdO 52700 2130 5.30 0.15 0.977 0.5323 0.0701 -11.539 0.013 0.021 0.120 0.018 0.014 100.8 37.9 26.0 0.11 0.06 0.04 +SDSSJ061510.23+355117.2 3452919960980353920 sdB 29076 184 5.51 0.04 0.891 0.6433 0.0516 -11.319 0.012 0.011 0.165 0.014 0.012 17.6 3.5 2.9 0.32 0.07 0.06 +SDSSJ061533.24+830110.5 1143749073667258240 sdB 24825 1160 5.28 0.16 0.226 1.0441 0.0267 -11.058 0.010 0.008 0.185 0.005 0.005 11.7 2.8 2.5 0.24 0.11 0.08 +SDSSJ061548.02+344650.2 3452646281368418304 sdB 25707 204 5.79 0.03 0.891 0.7985 0.0462 -11.191 0.031 0.010 0.179 0.011 0.010 12.5 2.2 2.0 0.72 0.11 0.09 +SDSSJ061754.20+233753.0 3425561981379261184 sdOB 38338 260 5.95 0.04 0.933 1.0084 0.0341 -11.184 0.019 0.010 0.143 0.005 0.005 39.6 3.3 3.1 0.66 0.08 0.07 +SDSSJ061927.52+352257.5 3452740362628172160 sdOB 37286 346 5.29 0.03 0.759 0.7353 0.0339 -11.163 0.013 0.013 0.208 0.010 0.009 75.3 8.1 7.1 0.31 0.04 0.04 +SDSSJ062704.91+345809.6 942463434178440576 sdB 26624 293 5.32 0.03 0.385 1.2037 0.0286 -11.019 0.024 0.013 0.176 0.005 0.004 14.0 1.7 1.7 0.24 0.03 0.03 +SDSSJ064229.22+370413.2 943819308110646144 sdOB 36631 893 5.80 0.13 0.407 1.0128 0.0423 -11.242 0.028 0.010 0.126 0.006 0.005 25.5 3.7 3.4 0.36 0.13 0.10 +SDSSJ065251.84+290023.3 887620515740571264 sdB 33230 196 5.62 0.04 0.164 0.9839 0.0387 -11.186 0.012 0.003 0.147 0.006 0.006 23.5 2.5 2.3 0.33 0.05 0.04 +SDSSJ070215.20+121753.4 3160836861727862400 sdB 26933 355 5.27 0.04 0.394 0.9351 0.0418 -11.067 0.012 0.009 0.204 0.010 0.009 19.6 2.6 2.4 0.28 0.04 0.04 +SDSSJ070240.50+114741.6 3160522848078571008 He-sdO 43401 201 5.67 0.05 0.209 0.3634 0.0499 -11.482 0.008 0.009 0.201 0.032 0.024 128.8 44.2 29.2 0.69 0.26 0.17 +SDSSJ070718.60+140058.3 3161497015379649280 sdOB 40737 234 5.97 0.03 0.033 0.7705 0.0555 -11.406 0.043 0.008 0.113 0.009 0.008 31.6 5.3 4.4 0.43 0.08 0.07 +SDSSJ072351.47+301916.5 885963418573729792 sdB 32693 87 5.79 0.02 0.157 1.3041 0.0534 -11.231 0.005 0.005 0.100 0.005 0.004 10.2 1.7 1.6 0.22 0.03 0.03 +SDSSJ072501.47+270318.3 872695092069071360 sdB 32331 140 6.00 0.03 0.232 0.6934 0.0622 -11.439 0.005 0.011 0.116 0.012 0.010 13.3 3.1 2.5 0.49 0.11 0.09 +SDSSJ072726.41+444837.0 973652013509753600 He-sdO 47570 2000 5.77 0.20 0.372 0.4460 0.0451 -11.494 0.039 0.009 0.160 0.018 0.015 117.4 36.2 26.7 0.55 0.36 0.22 +SDSSJ072824.72+414953.7 948767385313600128 He-sdOB 39563 230 5.74 0.06 0.417 0.4243 0.0456 -11.386 0.030 0.005 0.214 0.026 0.021 100.9 25.6 18.8 0.92 0.28 0.20 +SDSSJ073131.56+204524.6 864917013671899648 sdO 44021 683 5.98 0.07 0.066 0.6424 0.0542 -11.498 0.008 0.004 0.109 0.010 0.009 39.9 8.2 6.5 0.41 0.11 0.09 +SDSSJ073220.14+270408.5 872322087046515840 He-sdOB 39187 316 5.77 0.07 0.211 0.4750 0.0709 -11.565 0.006 0.009 0.127 0.022 0.017 34.3 13.2 8.5 0.35 0.15 0.10 +SDSSJ073323.77+174417.3 3170114884438433152 sdB 31065 396 6.32 0.13 0.507 0.4306 0.0685 -12.050 0.027 0.013 0.045 0.009 0.007 1.7 1.6 1.5 0.16 0.09 0.06 +SDSSJ073325.61+365257.6 898625493262383104 sdB 32972 106 5.92 0.02 0.136 1.2158 0.0402 -11.237 0.004 0.010 0.106 0.004 0.004 11.9 1.6 1.6 0.34 0.04 0.03 +SDSSJ073445.11+302949.5 879823195888098560 sdB 30211 481 5.33 0.10 0.068 0.5284 0.0600 -11.315 0.004 0.007 0.203 0.026 0.021 30.9 8.8 6.4 0.32 0.13 0.09 +SDSSJ073712.27+264224.7 872072016870129024 sdB 33039 449 5.51 0.08 0.933 0.6672 0.0363 -11.079 0.106 0.016 0.272 0.016 0.014 79.3 10.5 9.0 0.88 0.21 0.17 +SDSSJ073714.25+250554.6 868529562204066688 sdB 29336 278 5.52 0.05 0.080 0.4800 0.0450 -11.256 0.008 0.008 0.256 0.026 0.022 43.6 9.6 7.4 0.79 0.20 0.15 +SDSSJ074023.56+204937.0 673058556816796288 sdOB 33988 916 5.78 0.14 0.014 0.5818 0.0528 -11.382 0.005 0.005 0.158 0.016 0.013 30.0 7.4 5.7 0.55 0.25 0.17 +SDSSJ074552.59+255127.3 868817943488022016 sdB 26339 434 5.16 0.05 0.098 0.7626 0.0434 -11.100 0.008 0.007 0.231 0.014 0.012 23.0 3.6 3.1 0.28 0.05 0.05 +SDSSJ074603.33+334436.8 882125367078828672 sdB 27295 265 5.30 0.03 0.115 0.6062 0.0363 -11.141 0.007 0.010 0.264 0.017 0.015 34.8 5.0 4.2 0.51 0.08 0.07 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5.25 0.18 0.282 0.4562 0.0664 -11.478 0.019 0.010 0.161 0.028 0.021 10.6 4.8 3.3 0.17 0.12 0.07 +SDSSJ075134.21+092554.7 3148758039302713984 sdB 26596 1240 5.20 0.18 0.023 0.6130 0.0490 -11.304 0.007 0.016 0.180 0.016 0.014 14.6 4.3 3.5 0.19 0.11 0.07 +SDSSJ075154.72+133247.5 3152400171567834368 sdOB 35981 540 5.37 0.09 0.085 0.6550 0.0486 -11.426 0.004 0.030 0.127 0.010 0.009 24.4 4.6 3.8 0.14 0.05 0.04 +SDSSJ075227.28+194512.2 673296699867377024 sdB 28310 1096 5.56 0.16 0.091 0.5255 0.0937 -11.599 0.011 0.015 0.106 0.023 0.016 6.5 3.7 2.4 0.15 0.11 0.06 +SDSSJ075314.03+111240.1 3150707232898463616 sdB 30067 226 5.35 0.04 0.057 0.5042 0.0475 -11.314 0.016 0.006 0.213 0.022 0.018 33.3 7.5 5.8 0.37 0.09 0.07 +SDSSJ075354.22+253109.8 873767017124252544 sdB 34162 169 5.80 0.03 0.092 0.5620 0.0448 -11.384 0.008 0.017 0.163 0.014 0.012 32.3 6.0 4.8 0.61 0.12 0.10 +SDSSJ075412.38+294957.1 877431345781684480 sdB 32818 113 5.73 0.02 0.111 1.0881 0.0451 -11.133 0.006 0.006 0.149 0.007 0.006 23.3 2.5 2.3 0.44 0.05 0.04 +SDSSJ075603.77+222630.9 674255203425267584 sdO 51160 5270 5.73 0.26 0.164 1.0823 0.0445 -11.153 0.005 0.013 0.145 0.006 0.006 128.9 63.2 46.0 0.41 0.34 0.19 +SDSSJ075610.33+410453.6 922207131460711040 sdB 23961 838 5.70 0.10 0.046 0.5977 0.0789 -11.548 0.031 0.007 0.105 0.016 0.012 3.3 1.8 1.6 0.20 0.09 0.06 +SDSSJ075711.83+134508.4 654222239006166656 sdOB 36907 911 5.85 0.13 0.105 0.5669 0.0529 -11.467 0.018 0.005 0.133 0.014 0.011 29.6 7.3 5.6 0.46 0.20 0.14 +SDSSJ075944.98+371503.1 907291264093243520 He-sdOB 35063 167 5.99 0.04 0.108 0.5121 0.0554 -11.514 0.004 0.007 0.132 0.016 0.013 23.8 6.3 4.7 0.63 0.17 0.13 +SDSSJ080327.93+342140.7 905650346067635968 sdOB 39177 381 5.48 0.04 0.155 0.5845 0.0451 -11.320 0.008 0.008 0.181 0.015 0.013 69.5 12.5 10.0 0.36 0.08 0.06 +SDSSJ080628.65+242057.5 680914734899282560 sdB 27934 430 5.29 0.05 0.135 0.7281 0.0503 -11.168 0.010 0.014 0.207 0.015 0.013 23.4 4.1 3.5 0.31 0.06 0.05 +SDSSJ080758.25+272434.3 683766356962547840 sdOB 41481 224 5.56 0.02 0.050 0.7640 0.0512 -11.149 0.008 0.010 0.207 0.015 0.013 113.7 17.2 14.0 0.57 0.09 0.08 +SDSSJ080921.96+160841.2 656428099850193664 sdOB 36316 967 5.63 0.13 0.112 0.4329 0.0447 -11.441 0.023 0.004 0.185 0.021 0.017 53.5 14.4 10.9 0.54 0.24 0.16 +SDSSJ081112.70+000131.2 3083502981967969664 sdB 28137 1016 5.60 0.15 0.015 1.1742 0.0449 -10.940 0.010 0.006 0.217 0.009 0.008 26.5 4.8 4.3 0.68 0.29 0.20 +SDSSJ081354.34-003833.6 3071397878637938304 sdB 27971 1160 5.44 0.17 0.188 0.5354 0.0514 -11.422 0.009 0.009 0.157 0.017 0.014 13.5 4.2 3.3 0.25 0.14 0.09 +SDSSJ081531.20+245222.6 682305655764689408 sdOB 38848 244 5.85 0.04 0.078 0.4487 0.0673 -11.537 0.041 0.005 0.143 0.025 0.019 41.8 15.9 10.3 0.53 0.21 0.14 +SDSSJ081959.61+224100.6 676607952150024448 sdB 32451 144 5.77 0.04 0.038 0.7930 0.0525 -11.352 0.008 0.007 0.123 0.009 0.008 15.2 2.7 2.3 0.33 0.06 0.05 +SDSSJ082053.53+000843.4 3077510098136276480 sdB 25800 290 5.52 0.04 0.151 0.6822 0.0477 -11.204 0.007 0.016 0.205 0.015 0.013 16.7 3.1 2.6 0.51 0.10 0.08 +SDSSJ082332.09+113641.9 649228871371933312 sdB 31200 600 5.79 0.06 0.017 0.5466 0.0863 -11.552 0.008 0.006 0.114 0.021 0.015 11.0 4.9 3.2 0.29 0.13 0.08 +SDSSJ082445.68+231520.3 678116344664890368 sdB 30455 139 5.62 0.03 0.050 0.6147 0.0550 -11.278 0.007 0.009 0.192 0.019 0.016 28.5 6.0 4.7 0.56 0.12 0.10 +SDSSJ083117.55-041433.3 3065764904474702720 sdB 32625 944 5.76 0.15 0.054 0.4637 0.0685 -11.538 0.007 0.008 0.139 0.024 0.018 19.6 8.0 5.3 0.41 0.24 0.15 +SDSSJ083211.98+122056.4 602793579048797312 sdOB 31372 449 5.21 0.07 0.136 1.1800 0.0360 -10.808 0.034 0.017 0.291 0.009 0.009 73.7 6.6 6.0 0.50 0.10 0.08 +SDSSJ083256.31-025537.9 3072637990315089024 sdB 27286 1239 5.23 0.18 0.093 0.4556 0.0628 -11.358 0.019 0.005 0.213 0.034 0.026 22.6 9.4 6.3 0.29 0.19 0.11 +SDSSJ083435.40+134336.9 603338210965969280 sdB 22762 1251 4.94 0.17 0.285 0.4257 0.0519 -11.276 0.011 0.010 0.276 0.038 0.030 18.4 7.3 5.2 0.24 0.14 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0.04 0.116 0.5919 0.0521 -11.384 0.023 0.023 0.155 0.015 0.013 26.6 5.5 4.4 0.58 0.13 0.10 +SDSSJ085042.50+024546.1 577999175230073728 sdB 25335 1216 5.23 0.17 0.234 0.4183 0.0482 -11.261 0.015 0.015 0.292 0.038 0.030 31.6 11.3 8.2 0.53 0.31 0.19 +SDSSJ085900.32+023313.1 577792849295295488 sdOB 33882 917 5.67 0.13 0.108 0.4337 0.0580 -11.485 0.011 0.015 0.168 0.026 0.020 33.3 11.9 8.1 0.48 0.25 0.16 +SDSSJ092206.80+081929.4 587484528898551552 sdOB 32803 917 5.81 0.13 0.126 0.7160 0.0588 -11.351 0.019 0.011 0.138 0.013 0.010 19.7 4.7 3.8 0.45 0.18 0.13 +SDSSJ092447.10+231917.6 639171814606295424 sdB 25652 826 5.35 0.10 0.351 0.4774 0.0529 -11.226 0.061 0.011 0.271 0.034 0.027 28.5 8.8 6.4 0.60 0.23 0.16 +SDSSJ092617.51+671853.7 1069105290840804480 sdOB 34833 934 5.72 0.14 0.437 0.4159 0.0576 -11.487 0.006 0.005 0.174 0.028 0.021 39.9 14.7 9.8 0.58 0.32 0.20 +SDSSJ095746.60+045448.6 3849270435091240192 sdB 27244 327 5.34 0.04 0.117 0.4502 0.0509 -11.210 0.004 0.010 0.305 0.039 0.031 45.9 12.7 9.1 0.74 0.22 0.16 +SDSSJ101342.12+260620.0 739156243780100352 sdO 61120 881 6.05 0.05 0.029 0.5181 0.0773 -11.652 0.018 0.005 0.095 0.017 0.012 113.8 44.1 27.8 0.37 0.15 0.10 +SDSSJ102844.63+253018.3 727435316684008832 sdO 42792 716 5.46 0.06 1.349 0.3664 0.0439 -11.283 0.091 0.018 0.305 0.041 0.033 279.7 84.0 58.7 0.98 0.33 0.23 +SDSSJ103854.02+525847.8 849277216680457600 sdB 26127 1191 5.31 0.17 0.038 0.3992 0.0539 -11.416 0.015 0.005 0.213 0.033 0.025 19.0 7.8 5.3 0.34 0.21 0.13 +SDSSJ105244.44+245925.3 729598330934052480 sdOB 33792 947 5.70 0.15 0.229 0.4234 0.0649 -11.574 0.041 0.008 0.140 0.025 0.018 22.8 9.6 6.2 0.36 0.22 0.13 +SDSSJ133040.91-001710.7 3638888712001832704 sdB 29545 344 5.90 0.08 0.019 0.5735 0.0676 -11.381 0.009 0.007 0.160 0.021 0.017 17.6 5.3 3.8 0.75 0.27 0.19 +SDSSJ133135.41+020919.8 3711881543758246144 sdOB 35600 300 5.72 0.06 0.135 0.4222 0.0814 -11.662 0.022 0.007 0.113 0.027 0.018 18.5 10.0 5.7 0.25 0.14 0.08 +SDSSJ134947.70+250810.9 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0.21 0.07 0.05 +SDSSJ153526.07+211441.0 1211366667953907328 He-sdOB 38000 2000 5.83 0.20 1.479 0.4128 0.0532 -11.423 0.065 0.030 0.190 0.028 0.022 67.9 27.4 18.9 0.90 0.63 0.36 +SDSSJ155041.99+294523.5 1320813464131916416 sdB 30422 820 5.60 0.10 0.093 0.3263 0.0458 -11.496 0.032 0.005 0.216 0.035 0.027 36.1 13.6 9.0 0.69 0.31 0.20 +SDSSJ155256.15+044158.7 4426133093259118336 sdOB 39753 994 5.77 0.12 0.226 0.3267 0.0639 -11.698 0.009 0.003 0.136 0.033 0.022 41.6 23.3 13.0 0.40 0.27 0.15 +SDSSJ155332.95+034434.4 4425177342776008832 sdOB 37387 1023 5.66 0.15 1.245 0.3559 0.0706 -11.400 0.146 0.020 0.238 0.058 0.039 99.9 56.8 31.6 0.96 0.71 0.38 +SDSSJ155628.34+011335.0 4410947978684680320 sdB 32700 600 5.51 0.08 0.427 0.3567 0.0628 -11.388 0.030 0.011 0.250 0.053 0.037 64.4 30.9 18.3 0.75 0.40 0.23 +SDSSJ155926.54+001440.4 4409987246040338816 sdB 32964 378 5.88 0.10 0.417 0.4569 0.0627 -11.443 0.039 0.007 0.174 0.028 0.021 32.2 11.2 7.5 0.85 0.38 0.25 +SDSSJ161437.93+231705.8 1301900627183028864 He-sdOB 37800 800 5.21 0.25 1.928 0.3587 0.0601 -11.393 0.068 0.035 0.233 0.046 0.033 99.3 44.7 27.4 0.33 0.31 0.16 +SDSSJ161921.70+295506.1 1318236621192489216 sdB 34115 933 5.79 0.15 0.124 0.3585 0.0569 -11.626 0.013 0.010 0.146 0.027 0.020 26.1 11.3 7.2 0.49 0.30 0.18 +SDSSJ162250.09+002631.9 4407832924803651584 sdB 29782 1047 5.51 0.16 0.275 0.4798 0.0760 -11.535 0.008 0.007 0.135 0.025 0.018 12.8 5.9 3.8 0.22 0.14 0.09 +SDSSJ162336.30+153236.5 4464184270115888768 sdOB 39148 970 5.97 0.16 0.596 0.4217 0.0650 -11.607 0.032 0.020 0.126 0.023 0.017 33.7 14.0 8.9 0.55 0.35 0.21 +SDSSJ163435.32+262101.7 1304379201270414592 sdO 43490 2624 5.79 0.17 0.832 0.3061 0.0532 -11.629 0.050 0.018 0.164 0.034 0.024 86.9 48.5 29.0 0.62 0.44 0.25 +SDSSJ163446.41+264146.6 1304442113951445120 sdB 34824 800 5.28 0.14 0.692 0.3803 0.0665 -11.559 0.055 0.015 0.160 0.033 0.024 33.7 16.2 9.7 0.18 0.12 0.07 +SDSSJ164122.32+334452.0 1326422863218478592 sdB 28200 500 5.49 0.11 0.072 0.5790 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0.10 +UVO0904-02 5762960596350664832 He-sdO 46200 250 5.64 0.05 0.025 1.9776 0.0574 -10.764 0.006 0.010 0.193 0.006 0.006 152.7 9.9 9.1 0.59 0.08 0.07 +UVO1735+22 4557081835745623808 sdOB 38000 500 5.54 0.05 0.126 2.3476 0.0464 -10.679 0.016 0.017 0.198 0.004 0.004 73.6 5.2 4.9 0.50 0.07 0.06 diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aasjournal.bst b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aasjournal.bst new file mode 100644 index 0000000..07b6944 --- /dev/null +++ b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aasjournal.bst @@ -0,0 +1,1801 @@ +%% AASJournal.bst June 3, 2019 +%% +%% Revision 1.18 2019/6/3 Amy Hendrickson +%% Took out `v' preceding version number in @misc +%% +%% Rewrote format.pid to implement this precedence: +%% if doi, print that, if eprint print that, if neither +%% and there is a url, use the url + +%% Took out format.url output generally because it is included in format.pid, +%% so undesirable to call for it a second time. + +%% +%% Revision 1.17 2019/3/15 Amy Hendrickson +%% Added DOI to every field where format.url was found. Kept format.url in case +%% it is needed. +%% + +%% Revision 1.16 2017/10/26 Amy Hendrickson +%% `url' only active when used in misc +%% +%% `note' is disabled in all cases; as is adsnote and adsurl. +%% +%% Repair to @misc call to aaspublisher to prevent `, ,' +%% when there is no publisher listed. +%% +%% Make correct hyperlinked content for doi, ascl, and arXiv; +%% changed definition of FUNCTION {format.eprint} to compare +%% archivePrefix with "arXiv" and when they match do +%% ' {new.block "\doarXiv{" eprint * "}" * } +%% otherwise do +%% ' {new.block "\doeprint{" eprint * "}" * } +%% +%% \dodoi, \doarXiv and \doeprint definitions are sent to the top of the .bbl file +%% with commands found in FUNCTION {begin.bib}. +%% +%% bbl.version no longer used, could be deleted. +%% +%% Version number is added when author enters: version = {number}, only in `misc' +%% +%% Removed `format.doi output' in {article} because in +%% combination with { format.pid output } we could get double doi entries +%% in the bibliography. +%% +%% Rewrote format.pid so that we can check to see if we have a doi number; in +%% which case we use that and suppress the arXiv and eprint combination. However, +%% we do Not eliminate the url field if the author has entered it. +%% +%% Deleted format.miscversion and made a simplified way to produce version in @misc +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%% Revision 1.15 2016/10/5 Amy Hendrickson +%% Changed bbl.version so that there is no longer a trailing `.' + +%% Revision 1.14 2016/9/14 Amy Hendrickson +%% Added URL field + +%% Revision 1.13 2016/8/9 Amy Hendrickson +%% Change to presort and bibsort to get multiple entries with same author/year +%% combination to be ordered in bibliography in same order as \cite{}s entered in text. + +%% Revision 1.12 2016/2/11 Amy Hendrickson +%% Changes to @misc function to specifications by Dr. August Muench. +%% Made comma appear between title and publisher whether or not there is a version number. + +%% Revision 1.11 2015/12/31 Amy Hendrickson +%% Changes to @misc function to specifications by Dr. August Muench. +%% Added version and publisher fields. + +%% Revision 1.10 2013/03/11 13:01:55 alberto +%% Reworked code to use format.pid for articles without proper +%% pagination which then leads the system to use either an eprint +%% id or a DOI; this will solve most problems with citing early +%% access articles (no volume of page available, but online). +%% Removed bibliography count from preamble since it seems to +%% confuse some versions of latex. +%% +%% Revision 1.9 2013/2/19 Erik Tollerud +%% fixes for spurious error messages due to rev 1.8 changes +%% also fixed missing publisher field printing in "book" +%% +%% Revision 1.8 2013/01/10 16:31:34 alberto +%% Added proper formatting of arXiv eprint entries output by ADS +%% (these are article records, but the eprint id is printed only +%% if no traditional page number is available). Also added support +%% for ASCL entries under the "misc" category. +%% +%% Revision 1.7 2011/11/21 13:10:12 alberto +%% Implemented new ApJ formatting rules: for papers with more than +%% 5 authors, print first 3 followed by "et al." +%% +%% Revision 1.6 2009/05/18 15:13:02 alberto +%% Fixed sorting of references with truncated lists of authors +%% in sort.format.names +%% Fix courtesy of Stephen Fegan +%% +%% Revision 1.5 2009/03/19 13:15:11 alberto +%% Truncate \bibitem entries with more than 8 authors. +%% Fix courtesy of Craig Wiegert +%% and Andrew R. Marble +%% +%% Revision 1.4 2002/06/18 16:37:48 alberto +%% Add comma after first author in two-author reference +%% Fix courtesy of Tim Robishaw +%% +%% Revision 1.3 2000/04/20 22:17:50 jbaker +%% Fixed INBOOK bug, now works essentially like BOOK. +%% +%% Revision 1.2 1998/08/30 22:35:45 jbaker +%% Added RCS keywords. +%% +%% 1998/08/12 J Baker +%% Tweaked by hand to get correct results for ApJ. Added functions from +%% astrobib. + + +%% +%% This originally was file `apj.bst', +%% generated with the docstrip utility. +%% +%% The original source files were: +%% +%% merlin.mbs (with options: `,ay,nat,nm-rev,nmdash,dt-beg,yr-per,note-yr,atit-u,jtit-x,jttl-rm,thtit-a,vnum-x,volp-com,jpg-1,pp-last,btit-rm,add-pub,pub-par,pre-edn,edby,edbyx,blk-com,fin-bare,ppx,ed,abr,ord,jabr,amper,em-x') +%% ---------------------------------------- +%% *** Bibliographic Style for ApJ *** +%% + %------------------------------------------------------------------- + % The original source file contains the following version information: + % \ProvidesFile{merlin.mbs}[1998/02/25 3.85a (PWD)] + % + % NOTICE: + % This file may be used for non-profit purposes. + % It may not be distributed in exchange for money, + % other than distribution costs. + % + % The author provides it `as is' and does not guarantee it in any way. + % + % Copyright (C) 1994-98 Patrick W. Daly + %------------------------------------------------------------------- + % For use with BibTeX version 0.99a or later + %------------------------------------------------------------------- + % This bibliography style file is intended for texts in ENGLISH + % This is an author-year citation style bibliography. As such, it is + % non-standard LaTeX, and requires a special package file to function properly. + % Such a package is natbib.sty by Patrick W. Daly + % The form of the \bibitem entries is + % \bibitem[Jones et al.(1990)]{key}... + % \bibitem[Jones et al.(1990)Jones, Baker, and Smith]{key}... + % The essential feature is that the label (the part in brackets) consists + % of the author names, as they should appear in the citation, with the year + % in parentheses following. There must be no space before the opening + % parenthesis! + % With natbib v5.3, a full list of authors may also follow the year. + % In natbib.sty, it is possible to define the type of enclosures that is + % really wanted (brackets or parentheses), but in either case, there must + % be parentheses in the label. + % The \cite command functions as follows: + % \citet{key} ==>> Jones et al. (1990) + % \citet*{key} ==>> Jones, Baker, and Smith (1990) + % \citep{key} ==>> (Jones et al., 1990) + % \citep*{key} ==>> (Jones, Baker, and Smith, 1990) + % \citep[chap. 2]{key} ==>> (Jones et al., 1990, chap. 2) + % \citep[e.g.][]{key} ==>> (e.g. Jones et al., 1990) + % \citep[e.g.][p. 32]{key} ==>> (e.g. Jones et al., p. 32) + % \citeauthor{key} ==>> Jones et al. + % \citeauthor*{key} ==>> Jones, Baker, and Smith + % \citeyear{key} ==>> 1990 + %--------------------------------------------------------------------- + +ENTRY + { address + archivePrefix + author + booktitle + chapter + doi + edition + editor + eprint + howpublished + institution + journal + key + month + number + organization + pages + publisher + school + series + title + misctitle + type + volume + year + version + url + } + {} + { label extra.label sort.label short.list } + +INTEGERS { output.state before.all mid.sentence after.sentence after.block } + +FUNCTION {init.state.consts} +{ #0 'before.all := + #1 'mid.sentence := + #2 'after.sentence := + #3 'after.block := +} + +STRINGS { s t } + +FUNCTION {output.nonnull} +{ 's := + output.state mid.sentence = + { ", " * write$ } + { output.state after.block = + { add.period$ write$ + newline$ + "\newblock " write$ + } + { output.state before.all = + 'write$ + { add.period$ " " * write$ } + if$ + } + if$ + mid.sentence 'output.state := + } + if$ + s +} + +FUNCTION {output} +{ duplicate$ empty$ + 'pop$ + 'output.nonnull + if$ +} + +FUNCTION {output.check} +{ 't := + duplicate$ empty$ + { pop$ "empty " t * " in " * cite$ * warning$ } + 'output.nonnull + if$ +} + +FUNCTION {fin.entry} +{ duplicate$ empty$ + 'pop$ + 'write$ + if$ + newline$ +} + +FUNCTION {new.block} +{ output.state before.all = + 'skip$ + { after.block 'output.state := } + if$ +} + +FUNCTION {new.sentence} +{ output.state after.block = + 'skip$ + { output.state before.all = + 'skip$ + { after.sentence 'output.state := } + if$ + } + if$ +} + +FUNCTION {add.blank} +{ " " * before.all 'output.state := +} + +FUNCTION {date.block} +{ + skip$ +} + +FUNCTION {not} +{ { #0 } + { #1 } + if$ +} + +FUNCTION {and} +{ 'skip$ + { pop$ #0 } + if$ +} + +FUNCTION {or} +{ { pop$ #1 } + 'skip$ + if$ +} + +FUNCTION {new.block.checkb} +{ empty$ + swap$ empty$ + and + 'skip$ + 'new.block + if$ +} + +FUNCTION {field.or.null} +{ duplicate$ empty$ + { pop$ "" } + 'skip$ + if$ +} + +FUNCTION {emphasize} +{ skip$ } + +FUNCTION {capitalize} +{ "u" change.case$ "t" change.case$ } + +FUNCTION {space.word} +{ " " swap$ * " " * } + + % Here are the language-specific definitions for explicit words. + % Each function has a name bbl.xxx where xxx is the English word. + % The language selected here is ENGLISH +FUNCTION {bbl.and} +{ "and"} + +FUNCTION {bbl.editors} +{ "eds." } + +FUNCTION {bbl.editor} +{ "ed." } + +FUNCTION {bbl.edby} +{ "edited by" } + +FUNCTION {bbl.edition} +{ "edn." } + +FUNCTION {bbl.volume} +{ "Vol." } + +FUNCTION {bbl.version} +{ "" } + +FUNCTION {bbl.of} +{ "of" } + +FUNCTION {bbl.number} +{ "no." } + +FUNCTION {bbl.nr} +{ "no." } + +FUNCTION {bbl.in} +{ "in" } + +FUNCTION {bbl.pages} +{ "" } + +FUNCTION {bbl.page} +{ "" } + +FUNCTION {bbl.chapter} +{ "Ch." } + +FUNCTION {bbl.techrep} +{ "Tech. Rep." } + +FUNCTION {bbl.mthesis} +{ "Master's thesis" } + +FUNCTION {bbl.phdthesis} +{ "PhD thesis" } + +FUNCTION {bbl.first} +{ "1st" } + +FUNCTION {bbl.second} +{ "2nd" } + +FUNCTION {bbl.third} +{ "3rd" } + +FUNCTION {bbl.fourth} +{ "4th" } + +FUNCTION {bbl.fifth} +{ "5th" } + +FUNCTION {bbl.st} +{ "st" } + +FUNCTION {bbl.nd} +{ "nd" } + +FUNCTION {bbl.rd} +{ "rd" } + +FUNCTION {bbl.th} +{ "th" } + +MACRO {jan} {"Jan."} + +MACRO {feb} {"Feb."} + +MACRO {mar} {"Mar."} + +MACRO {apr} {"Apr."} + +MACRO {may} {"May"} + +MACRO {jun} {"Jun."} + +MACRO {jul} {"Jul."} + +MACRO {aug} {"Aug."} + +MACRO {sep} {"Sep."} + +MACRO {oct} {"Oct."} + +MACRO {nov} {"Nov."} + +MACRO {dec} {"Dec."} + +FUNCTION {eng.ord} +{ duplicate$ "1" swap$ * + #-2 #1 substring$ "1" = + { bbl.th * } + { duplicate$ #-1 #1 substring$ + duplicate$ "1" = + { pop$ bbl.st * } + { duplicate$ "2" = + { pop$ bbl.nd * } + { "3" = + { bbl.rd * } + { bbl.th * } + if$ + } + if$ + } + if$ + } + if$ +} + +INTEGERS { nameptr namesleft numnames numtrunc } + +FUNCTION {format.names} +{ 's := + #0 'numtrunc := + #1 'nameptr := + s num.names$ 'numnames := + numnames 'namesleft := + numnames #5 > + { #3 'numtrunc := } + {} + if$ + { namesleft #0 > } + { s nameptr + "{vv~}{ll}{, jj}{, f.}" format.name$ + 't := + nameptr #1 > + { + nameptr #1 - numtrunc = + { + #1 'namesleft := + "others" 't := + } + {} + if$ + + namesleft #1 > + { ", " * t * } + { + numnames #1 > + { "," * } + 'skip$ + if$ + s nameptr "{ll}" format.name$ duplicate$ "others" = + { 't := } + { pop$ } + if$ + t "others" = + { + " {et~al.}" * + } + { " \& " * t * } + if$ + } + if$ + } + 't + if$ + nameptr #1 + 'nameptr := + namesleft #1 - 'namesleft := + } + while$ +} + +FUNCTION {format.names.ed} +{ 's := + #1 'nameptr := + s num.names$ 'numnames := + numnames 'namesleft := + { namesleft #0 > } + { s nameptr + "{f.~}{vv~}{ll}{, jj}" + format.name$ + 't := + nameptr #1 > + { + namesleft #1 > + { ", " * t * } + { + numnames #2 > + { "," * } + 'skip$ + if$ + s nameptr "{ll}" format.name$ duplicate$ "others" = + { 't := } + { pop$ } + if$ + t "others" = + { + " {et~al.}" * + } + { " \& " * t * } + if$ + } + if$ + } + 't + if$ + nameptr #1 + 'nameptr := + namesleft #1 - 'namesleft := + } + while$ +} + +FUNCTION {format.key} +{ empty$ + { key field.or.null } + { "" } + if$ +} + +FUNCTION {format.authors} +{ author empty$ + { "" } + { author format.names } + if$ +} + +FUNCTION {format.editors} +{ editor empty$ + { "" } + { editor format.names + editor num.names$ #1 > + { ", " * bbl.editors * } + { ", " * bbl.editor * } + if$ + } + if$ +} + +FUNCTION {format.in.editors} +{ editor empty$ + { "" } + { editor format.names.ed + } + if$ +} + + +FUNCTION {format.title} +{ title empty$ + { "" } + { title + } + if$ +} + +FUNCTION {format.full.names} +{'s := + #1 'nameptr := + s num.names$ 'numnames := + numnames 'namesleft := + { namesleft #0 > } + { s nameptr + "{vv~}{ll}" format.name$ + 't := + nameptr #1 > + { + namesleft #1 > + { ", " * t * } + { + numnames #2 > + { "," * } + 'skip$ + if$ + s nameptr "{ll}" format.name$ duplicate$ "others" = + { 't := } + { pop$ } + if$ + t "others" = + { + " {et~al.}" * + } + { " \& " * t * } + if$ + } + if$ + } + 't + if$ + nameptr #1 + 'nameptr := + namesleft #1 - 'namesleft := + } + while$ +} + +FUNCTION {author.editor.key.full} +{ author empty$ + { editor empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { editor format.full.names } + if$ + } + { author format.full.names } + if$ +} + +FUNCTION {author.key.full} +{ author empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { author format.full.names } + if$ +} + +FUNCTION {editor.key.full} +{ editor empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { editor format.full.names } + if$ +} + +FUNCTION {make.full.names} +{ type$ "book" = + type$ "inbook" = + or + 'author.editor.key.full + { type$ "proceedings" = + 'editor.key.full + 'author.key.full + if$ + } + if$ +} + +FUNCTION {output.bibitem} +{ newline$ + "\bibitem[{" write$ + label write$ + ")" make.full.names duplicate$ short.list = + { pop$ } + { * } + if$ + "}]{" * write$ + cite$ write$ + "}" write$ + newline$ + "" + before.all 'output.state := +} + + +FUNCTION {format.url} +{ url empty$ + { "" } + { new.block "\url{" url * "}" * } + if$ +} + +FUNCTION {format.eprint} +{ eprint empty$ + { "" } + { archivePrefix empty$ + { "" } + { archivePrefix "arXiv" = + {new.block "\doarXiv{" eprint * "}" * } + {new.block "\doeprint{" eprint * "}" * } + if$} + if$ + } + if$ +} + +% Formats a persistent identifier (PID) +% (typically a DOI or an eprint id) +% You can easily swap the order of which PID +% gets picked +% + +FUNCTION {format.doi} +{ doi empty$ + { "" } + { "\dodoi{" doi * "}" * } + if$ +} + +FUNCTION {format.pid} +{ doi empty$ +{eprint empty$ + { url empty$ + { "" } + { format.url } + if$} + { format.eprint } + if$} + { format.doi } + if$ +} + +FUNCTION {n.dashify} +{ + 't := + "" + { t empty$ not } + { t #1 #1 substring$ "-" = + { t #1 #2 substring$ "--" = not + { "--" * + t #2 global.max$ substring$ 't := + } + { { t #1 #1 substring$ "-" = } + { "-" * + t #2 global.max$ substring$ 't := + } + while$ + } + if$ + } + { t #1 #1 substring$ * + t #2 global.max$ substring$ 't := + } + if$ + } + while$ +} + +FUNCTION {word.in} +{ bbl.in + " " * } + +FUNCTION {format.date} +{ year duplicate$ empty$ + { "empty year in " cite$ * "; set to ????" * warning$ + pop$ "????" } + 'skip$ + if$ + extra.label * + before.all 'output.state := + after.sentence 'output.state := +} + +FUNCTION {format.btitle} +{ title +} + +FUNCTION {tie.or.space.connect} +{ duplicate$ text.length$ #3 < + { "~" } + { " " } + if$ + swap$ * * +} + +FUNCTION {either.or.check} +{ empty$ + 'pop$ + { "can't use both " swap$ * " fields in " * cite$ * warning$ } + if$ +} + +FUNCTION {format.bvolume} +{ volume empty$ + { "" } + { bbl.volume volume tie.or.space.connect + series empty$ + 'skip$ + { bbl.of space.word * series emphasize * } + if$ + "volume and number" number either.or.check + } + if$ +} + +FUNCTION {format.number.series} +{ volume empty$ + { number empty$ + { series field.or.null } + { output.state mid.sentence = + { bbl.number } + { bbl.number capitalize } + if$ + number tie.or.space.connect + series empty$ + { "there's a number but no series in " cite$ * warning$ } + { bbl.in space.word * series * } + if$ + } + if$ + } + { "" } + if$ +} + +FUNCTION {is.num} +{ chr.to.int$ + duplicate$ "0" chr.to.int$ < not + swap$ "9" chr.to.int$ > not and +} + +FUNCTION {extract.num} +{ duplicate$ 't := + "" 's := + { t empty$ not } + { t #1 #1 substring$ + t #2 global.max$ substring$ 't := + duplicate$ is.num + { s swap$ * 's := } + { pop$ "" 't := } + if$ + } + while$ + s empty$ + 'skip$ + { pop$ s } + if$ +} + +FUNCTION {convert.edition} +{ edition extract.num "l" change.case$ 's := + s "first" = s "1" = or + { bbl.first 't := } + { s "second" = s "2" = or + { bbl.second 't := } + { s "third" = s "3" = or + { bbl.third 't := } + { s "fourth" = s "4" = or + { bbl.fourth 't := } + { s "fifth" = s "5" = or + { bbl.fifth 't := } + { s #1 #1 substring$ is.num + { s eng.ord 't := } + { edition 't := } + if$ + } + if$ + } + if$ + } + if$ + } + if$ + } + if$ + t +} + +FUNCTION {format.edition} +{ edition empty$ + { "" } + { output.state mid.sentence = + { convert.edition "l" change.case$ " " * bbl.edition * } + { convert.edition "t" change.case$ " " * bbl.edition * } + if$ + } + if$ +} + +INTEGERS { multiresult } + +FUNCTION {multi.page.check} +{ 't := + #0 'multiresult := + { multiresult not + t empty$ not + and + } + { t #1 #1 substring$ + duplicate$ "-" = + swap$ duplicate$ "," = + swap$ "+" = + or or + { #1 'multiresult := } + { t #2 global.max$ substring$ 't := } + if$ + } + while$ + multiresult +} + +FUNCTION {format.pages} +{ pages empty$ + { "" } + { pages multi.page.check +% { bbl.pages pages n.dashify tie.or.space.connect } +% { bbl.page pages tie.or.space.connect } + { pages n.dashify } + { pages } + if$ + } + if$ +} + +FUNCTION {first.page} +{ 't := + "" + { t empty$ not t #1 #1 substring$ "-" = not and } + { t #1 #1 substring$ * + t #2 global.max$ substring$ 't := + } + while$ +} + +FUNCTION {format.journal.pages} +{ pages empty$ + 'skip$ + { duplicate$ empty$ + { pop$ format.pages } + { + ", " * + pages first.page * + } + if$ + } + if$ +} + + +FUNCTION {format.vol.num.pages} +{ volume field.or.null +} + +FUNCTION {format.chapter.pages} +{ chapter empty$ + { "" } + { type empty$ + { bbl.chapter } + { type "l" change.case$ } + if$ + chapter tie.or.space.connect + } + if$ +} + +FUNCTION {format.in.ed.booktitle} +{ booktitle empty$ + { "" } + { editor empty$ + { word.in booktitle emphasize * } + { word.in booktitle emphasize * + ", " * + editor num.names$ #1 > + { bbl.editors } + { bbl.editor } + if$ + * " " * + format.in.editors * + } + if$ + } + if$ +} + +FUNCTION {format.thesis.type} +{ type empty$ + 'skip$ + { pop$ + type "t" change.case$ + } + if$ +} + +FUNCTION {format.tr.number} +{ type empty$ + { bbl.techrep } + 'type + if$ + number empty$ + { "t" change.case$ } + { number tie.or.space.connect } + if$ +} + +FUNCTION {format.article.crossref} +{ + word.in + " \cite{" * crossref * "}" * +} + +FUNCTION {format.book.crossref} +{ volume empty$ + { "empty volume in " cite$ * "'s crossref of " * crossref * warning$ + word.in + } + { bbl.volume volume tie.or.space.connect + bbl.of space.word * + } + if$ + " \cite{" * crossref * "}" * +} + +FUNCTION {format.incoll.inproc.crossref} +{ + word.in + " \cite{" * crossref * "}" * +} + +FUNCTION {format.publisher} +{ publisher empty$ + { "empty publisher in " cite$ * warning$ } + 'skip$ + if$ + "" + address empty$ publisher empty$ and + 'skip$ + { + add.blank "(" * + address empty$ + 'skip$ + { address * } + if$ + publisher empty$ + 'skip$ + { address empty$ + 'skip$ + { ": " * } + if$ + publisher * + } + if$ + ")" * + } + if$ + output +} + +FUNCTION {format.aaspublisher} +{ publisher empty$ + { "empty publisher in " cite$ * warning$ } + 'skip$ + if$ + ", " + address empty$ publisher empty$ and + 'skip$ + { + add.blank "" * + address empty$ + 'skip$ + { address * } + if$ + publisher empty$ + 'skip$ + { address empty$ + 'skip$ + { ": " * } + if$ + publisher * + } + if$ + "" * + } + if$ + output +} + + + +STRINGS {oldname} + +FUNCTION {name.or.dash} +{ 's := + oldname empty$ + { s 'oldname := s } + { s oldname = + { "---" } + { s 'oldname := s } + if$ + } + if$ +} + +%%%%%%%% Functions added from astrobib + +FUNCTION {format.edn.btitle} % Title should be on stack. +{ duplicate$ empty$ edition empty$ or + 'skip$ + { ", " * format.edition * } + if$ +} + +FUNCTION {format.ed.booktitle} % The title should be on the stack. +{ duplicate$ empty$ + { "no book title in " cite$ * warning$ "" pop$ } + { editor empty$ + author empty$ or % Empty author means editor already given. + 'format.edn.btitle + { format.edn.btitle ", " * bbl.editor * " " * format.in.editors * } + if$ + } + if$ +} + +FUNCTION {format.full.book.spec} % The title should be on the stack. +{ series empty$ + { format.ed.booktitle + volume empty$ + { number empty$ + 'skip$ + { " there's a number but no series in " cite$ * warning$ + " No." number tie.or.space.connect * } + if$ + } + { ", Vol." volume tie.or.space.connect * + number empty$ + 'skip$ + {"Both volume and number fields in " * cite$ * warning$ } + if$ + } + if$ + } + { volume empty$ + { format.ed.booktitle ", " * series * + number empty$ + 'skip$ + { " No." number tie.or.space.connect * } + if$ + } + { series ", Vol." volume tie.or.space.connect * + ", " * swap$ format.ed.booktitle * + number empty$ + 'skip$ + {"Both volume and number fields in " * cite$ * warning$ } + if$ + } + if$ + } + if$ +} + +%%%%%%% End of functions from astrobib + +FUNCTION {article} +{ output.bibitem + format.authors "author" output.check + author format.key output + name.or.dash + format.date "year" output.check + date.block + crossref missing$ + { journal + "journal" output.check + format.vol.num.pages output + } + { format.article.crossref output.nonnull + format.pages output + } + if$ + pages empty$ + 'skip$ + { format.journal.pages } + if$ + format.pid output + fin.entry +} + +FUNCTION {book} +{ output.bibitem + author empty$ + { format.editors "author and editor" output.check + editor format.key output + name.or.dash + } + { format.authors output.nonnull + name.or.dash + crossref missing$ + { "author and editor" editor either.or.check } + 'skip$ + if$ + } + if$ + format.date "year" output.check + date.block + title format.full.book.spec output +% format.btitle "title" output.check +% crossref missing$ +% { format.bvolume output +% format.number.series output +% format.edition output + format.publisher +% } +% { +% format.book.crossref output.nonnull +% } +% if$ + format.pages output + format.pid output + fin.entry +} + +FUNCTION {booklet} +{ output.bibitem + format.authors output + author format.key output + name.or.dash + format.date "year" output.check + date.block + format.title "title" output.check + howpublished output + address output + format.pid output + fin.entry +} + +FUNCTION {inbook} +{ output.bibitem + author empty$ + { format.editors "author and editor" output.check + editor format.key output + name.or.dash + } + { format.authors output.nonnull + name.or.dash + crossref missing$ + { "author and editor" editor either.or.check } + 'skip$ + if$ + } + if$ + format.date "year" output.check + date.block + title format.full.book.spec output +% format.btitle "title" output.check +% crossref missing$ +% { +% format.bvolume output +% format.chapter.pages "chapter and pages" output.check +% format.number.series output +% format.edition output + format.publisher +% } +% { +% format.chapter.pages "chapter and pages" output.check +% format.book.crossref output.nonnull +% } +% if$ + format.pages "pages" output.check + format.pid output + fin.entry +} + +FUNCTION {incollection} +{ output.bibitem + format.authors "author" output.check + author format.key output + name.or.dash + format.date "year" output.check + date.block + bbl.in " " * booktitle format.full.book.spec * output +% crossref missing$ +% { format.in.ed.booktitle "booktitle" output.check +% format.bvolume output +% format.number.series output +% format.edition output +% format.chapter.pages output + format.publisher +% } +% { format.incoll.inproc.crossref output.nonnull +% format.chapter.pages output +% } +% if$ + format.pages "pages" output.check + format.pid output + fin.entry +} + +FUNCTION {inproceedings} +{ output.bibitem + format.authors "author" output.check + author format.key output % added + format.date "year" output.check + date.block + bbl.in " " * booktitle format.full.book.spec * output +% crossref missing$ +% { format.in.ed.booktitle "booktitle" output.check +% format.bvolume output +% format.number.series output + publisher empty$ + { organization output + address output + } + { organization output + format.publisher + } + if$ +% } +% { format.incoll.inproc.crossref output.nonnull +% } +% if$ + format.pages output + format.pid output + fin.entry +} + +FUNCTION {conference} { inproceedings } + + +FUNCTION {manual} +{ output.bibitem + format.authors output + author format.key output + name.or.dash + format.date "year" output.check + date.block + format.btitle "title" output.check + format.edition output + organization output + address output + format.pid output + fin.entry +} + +FUNCTION {mastersthesis} +{ output.bibitem + format.authors "author" output.check + author format.key output + name.or.dash + format.date "year" output.check + date.block +% format.title "title" output.check + bbl.mthesis format.thesis.type output.nonnull + school "school" output.check + address output + format.pid output + fin.entry +} + +FUNCTION {misc} +{output.bibitem + format.authors output + author format.key output + name.or.dash + format.date "year" output.check + date.block +%% new + format.title output +%% new + version empty$ + 'skip$ + {bbl.version version * output} + if$ +%% + howpublished output + publisher empty$ + {} + {format.aaspublisher} + if$ + format.pid output + fin.entry +} + +FUNCTION {phdthesis} +{ output.bibitem + format.authors "author" output.check + author format.key output + name.or.dash + format.date "year" output.check + date.block +% format.title "title" output.check + bbl.phdthesis format.thesis.type output.nonnull + school "school" output.check + address output + format.pid output + fin.entry +} + +FUNCTION {proceedings} +{ output.bibitem + editor empty$ + { organization output + organization format.key output } + { format.editors output } + if$ +% format.editors output +% editor format.key output + name.or.dash + format.date "year" output.check + date.block + title format.full.book.spec output +% format.btitle "title" output.check +% format.bvolume output +% format.number.series output + publisher empty$ not % No need for warning if no pub. + { format.publisher } + { editor empty$ % For empty editor, organization was already given. + 'skip$ + { organization output } + if$ + address output + } + if$ +% address output +% organization output +% publisher output + format.pages output + format.pid output + fin.entry +} + +FUNCTION {techreport} +{ output.bibitem + format.authors "author" output.check + author format.key output + name.or.dash + format.date "year" output.check + date.block + format.title "title" output.check + format.tr.number output.nonnull + institution "institution" output.check + address output + format.pid output + fin.entry +} + +FUNCTION {unpublished} +{ output.bibitem + format.authors "author" output.check + author format.key output + name.or.dash + format.date "year" output.check + date.block +% format.title "title" output.check + format.pid output + fin.entry +} + +FUNCTION {default.type} { misc } + +READ + +FUNCTION {sortify} +{ purify$ + "l" change.case$ +} + +INTEGERS { len } + +FUNCTION {chop.word} +{ 's := + 'len := + s #1 len substring$ = + { s len #1 + global.max$ substring$ } + 's + if$ +} + +FUNCTION {format.lab.names} +{ 's := + s #1 "{vv~}{ll}" format.name$ + s num.names$ duplicate$ + #2 > + { pop$ + " {et~al.}" * + } + { #2 < + 'skip$ + { s #2 "{ff }{vv }{ll}{ jj}" format.name$ "others" = + { + " {et~al.}" * + } + { " \& " * s #2 "{vv~}{ll}" format.name$ + * } + if$ + } + if$ + } + if$ +} + +FUNCTION {author.key.label} +{ author empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { author format.lab.names } + if$ +} + +FUNCTION {author.editor.key.label} +{ author empty$ + { editor empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { editor format.lab.names } + if$ + } + { author format.lab.names } + if$ +} + +FUNCTION {editor.key.label} +{ editor empty$ + { key empty$ + { cite$ #1 #3 substring$ } + 'key + if$ + } + { editor format.lab.names } + if$ +} + +FUNCTION {calc.short.authors} +{ type$ "book" = + type$ "inbook" = + or + 'author.editor.key.label + { type$ "proceedings" = + 'editor.key.label + 'author.key.label + if$ + } + if$ + 'short.list := +} + +FUNCTION {calc.label} +{ calc.short.authors + short.list + "(" + * + year duplicate$ empty$ + { pop$ "????" } + 'skip$ + if$ + * + 'label := +} + +FUNCTION {sort.format.names} +{ 's := + #1 'nameptr := + "" + s num.names$ 'numnames := + numnames #8 > + { s nameptr + "{vv{ } }{ll{ }}{ f{ }}{ jj{ }}" + format.name$ 't := + t sortify * + " " * + "zzzzz" * + } + { numnames 'namesleft := + { namesleft #0 > } + { s nameptr + "{vv{ } }{ll{ }}{ f{ }}{ jj{ }}" + format.name$ 't := + nameptr #1 > + { + " " * + namesleft #1 = t "others" = and + { "zzzzz" * } + { t sortify * } + if$ + } + { t sortify * } + if$ + nameptr #1 + 'nameptr := + namesleft #1 - 'namesleft := + } + while$ + } + if$ +} + +FUNCTION {sort.format.title} +{ 't := + "A " #2 + "An " #3 + "The " #4 t chop.word + chop.word + chop.word + sortify + #1 global.max$ substring$ +} + +FUNCTION {author.sort} +{ author empty$ + { key empty$ + { "to sort, need author or key in " cite$ * warning$ + "" + } + { key sortify } + if$ + } + { author sort.format.names } + if$ +} + +FUNCTION {author.editor.sort} +{ author empty$ + { editor empty$ + { key empty$ + { "to sort, need author, editor, or key in " cite$ * warning$ + "" + } + { key sortify } + if$ + } + { editor sort.format.names } + if$ + } + { author sort.format.names } + if$ +} + +FUNCTION {editor.sort} +{ editor empty$ + { key empty$ + { "to sort, need editor or key in " cite$ * warning$ + "" + } + { key sortify } + if$ + } + { editor sort.format.names } + if$ +} + +FUNCTION {presort} +{ calc.label + label sortify + " " + * + type$ "book" = + type$ "inbook" = + or + 'author.editor.sort + { type$ "proceedings" = + 'editor.sort + 'author.sort + if$ + } + if$ + #1 entry.max$ substring$ + 'sort.label := + sort.label + * + " " + * +%% August 2016 +%% commenting out this combination gets the cites right but references wrong +%% title field.or.null +%% sort.format.title +%% * +%% +%% with only this line on, we get cites right but references wrong + sort.format.title + #1 entry.max$ substring$ + 'sort.key$ := +} + +ITERATE {presort} + +SORT + +STRINGS { last.label next.extra } + +INTEGERS { last.extra.num number.label } + +FUNCTION {initialize.extra.label.stuff} +{ #0 int.to.chr$ 'last.label := + "" 'next.extra := + #0 'last.extra.num := + #0 'number.label := +} + +FUNCTION {forward.pass} +{ last.label label = + { last.extra.num #1 + 'last.extra.num := + last.extra.num int.to.chr$ 'extra.label := + } + { "a" chr.to.int$ 'last.extra.num := + "" 'extra.label := + label 'last.label := + } + if$ + number.label #1 + 'number.label := +} + +FUNCTION {reverse.pass} +{ next.extra "b" = + { "a" 'extra.label := } + 'skip$ + if$ + extra.label 'next.extra := + extra.label + duplicate$ empty$ + 'skip$ + { "{\natexlab{" swap$ * "}}" * } + if$ + 'extra.label := + label extra.label * 'label := +} + +EXECUTE {initialize.extra.label.stuff} + +ITERATE {forward.pass} + +REVERSE {reverse.pass} + +FUNCTION {bib.sort.order} +{ sort.label + " " + * + year field.or.null sortify + * + " " + * +%% Commented out August 2016, so that multiple indentical author/year +%% combinations are entered in the order that \cite{}s are found in text. +% title field.or.null +% sort.format.title +% * + #1 entry.max$ substring$ + 'sort.key$ := +} + +ITERATE {bib.sort.order} + +SORT + +FUNCTION {begin.bib} +{ preamble$ empty$ + 'skip$ + { preamble$ write$ newline$ } + if$ + "\begin{thebibliography}{}" + write$ newline$ + "\expandafter\ifx\csname natexlab\endcsname\relax\def\natexlab#1{#1}\fi" + write$ newline$ + "\providecommand{\url}[1]{\href{#1}{#1}}" + write$ newline$ + "\providecommand{\dodoi}[1]{doi:~\href{http://doi.org/#1}{\nolinkurl{#1}}}" + write$ newline$ + "\providecommand{\doeprint}[1]{\href{http://ascl.net/#1}{\nolinkurl{http://ascl.net/#1}}}" + write$ newline$ + "\providecommand{\doarXiv}[1]{\href{https://arxiv.org/abs/#1}{\nolinkurl{https://arxiv.org/abs/#1}}}" + write$ newline$ +} + + +EXECUTE {begin.bib} + +EXECUTE {init.state.consts} + +ITERATE {call.type$} + +FUNCTION {end.bib} +{ newline$ + "\end{thebibliography}" write$ newline$ +} + +EXECUTE {end.bib} +%% End of customized bst file +%% +%% End of file `aasjournal.bst'. \ No newline at end of file diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aastex631.cls b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aastex631.cls new file mode 100644 index 0000000..1b30c0e --- /dev/null +++ b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/aastex631.cls @@ -0,0 +1,7806 @@ +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% AASTEX631.cls %% +%% Jan 29f, 2021 %% +%% %% +%% Copyright 2021 American Astronomical Society %% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +\def\currversion{6.3.1f} + +%% +%% These files are distributed +%% WITHOUT ANY WARRANTY; without even the implied warranty of +%% MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. +%% +%% \CharacterTable +%% {Upper-case \A\B\C\D\E\F\G\H\I\J\K\L\M\N\O\P\Q\R\S\T\U\V\W\X\Y\Z +%% Lower-case \a\b\c\d\e\f\g\h\i\j\k\l\m\n\o\p\q\r\s\t\u\v\w\x\y\z +%% Digits \0\1\2\3\4\5\6\7\8\9 +%% Exclamation \! Double quote \" Hash (number) \# +%% Dollar \$ Percent \% Ampersand \& +%% Acute accent \' Left paren \( Right paren \) +%% Asterisk \* Plus \+ Comma \, +%% Minus \- Point \. Solidus \/ +%% Colon \: Semicolon \; Less than \< +%% Equals \= Greater than \> Question mark \? +%% Commercial at \@ Left bracket \[ Backslash \\ +%% Right bracket \] Circumflex \^ Underscore \_ +%% Grave accent \` Left brace \{ Vertical bar \| +%% Right brace \} Tilde \~}% +%% +%%% date = "9/19/2016", +%%% author = "Amy Hendrickson (mailto:amyh@texnology.com)" +%%% including +%%% 1) code from emulateapj.cls, version 01/23/15(marked below) +%%% written by Alexey Vikhlinin, which relies on RevTeX4-1 +%%% for much functionality; +%%% 2) some code from aastex (marked below) +%%% 3) Original work by Amy Hendrickson (marked below) for +%%% extensive table tools, including easy decimal entry and splitting +%%% tables horizontally into 2 or 3 pieces, for tabular and deluxetable +%%% environments; rotate tables; gridlines for use in positioning figures, +%%% track changes. + +%%% This work may be distributed and/or modified under the +%%% conditions of the LaTeX Project Public License, either version 1.3c +%%% of this license or (at your option) any later version. +%%% The latest version of this license is in +%%% http://www.latex-project.org/lppl.txt +%%% and version 1.3 or later is part of all distributions of LaTeX +%%% version 2005/12/01 or later. +% +%%% This work has the LPPL maintenance status `maintained'. +% +%%% The Current Maintainer of this work is Greg Schwarz +%%% This work consists of the file aastex.cls + +%%% copyright = "Copyright (C) 2016--2020 American Astronomical Society +%%% +%%% This work may be distributed and/or modified under the +%%% conditions of the LaTeX Project Public License, either version 1.3 +%%% of this license or (at your option) any later version. +%%% The latest version of this license is in +%%% http://www.latex-project.org/lppl.txt +%%% and version 1.3 or later is part of all distributions of LaTeX +%%% version 2003/12/01 or later. +%%% +%%% This work has the LPPL maintenance status "maintained". +%%% +%%% The Current Maintainer of this work is the American Astronomical Society. +%%% +%%% This work consists of all files listed in the document README. +%%% +%%% address = "American Astronomical Society +%%% USA", +%%% telephone = "+1 ???", +%%% FAX = "", +%%% email = "aastex-help@aas.org", +%%% codetable = "ISO/ASCII", +%%% keywords = "latex, AAS, journal", +%%% supported = "yes", +%%% abstract = "formatter for AAS journal submissions", +%%% } + + +\ProvidesClass{aastex631}%%% + [2020/12/20 Version 6.3.1d/AAS markup document class]% +{} +\ClassInfo{aastex}{% +^^J +^^J + Original \protect\LaTeX2.09 style + by Chris Biemesderfer (chris@seagoat.com). +^^J + Adapted to \protect\LaTeXe\space + by A. Ogawa (ogawa@teleport.com)% +^^J +emulateapj.cls included, Copyright 2000-2015 Alexey Vikhlinin +^^J +Rewrite and update of emulateapj.cls, +revised and enhanced with table macros, gridlines, draft watermark,^^J +track changes, new `modern' style and much more, by Amy Hendrickson,% +^^J + (amyh@texnology.com, http://www.texnology.com) +^^J +^^J +}% + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% aastex.cls version 2.0 is a based on emulateapj.cls, version January 23, 2015, +%% and an older version of aastex.cls, with many additional functionalities. +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%% Options. Document style options, and additional feature options. + +% These are the General document style options, 6 choices + +% manuscript : onecolumn, doublespace, 12pt fonts + +%% Preprints are like manuscript, except they are single spaced. +% preprint : onecolumn, single space, 12pt fonts +% preprint2 : twocolumn, single space, 12pt fonts + +%% Modern is new design developed by David Hogg and Daniel Foreman-Mackey +% modern : one column, single space, 12pt fonts, more stylish + +% twocolumn : a two column article, single space, 10pt fonts + +% Default document style option +% onecolumn : a one column article; single space, 10pt fonts + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Additional feature options: + +% revtex4 : will produce an error message and demand to download revtex4-1. +% twocolappendix: make 2 column appendix // produces error message. +% onecolappendix: make 1 column appendix is the default. // not needed because it is the default +% astrosymb : Loads Astrosymb font and define \astro commands. +% tighten : Makes baselineskip slightly smaller, only works with twocolumn option. +%% author can also use the commands \tighten, or \singlespace or \doublespace in the body of their article +%% to get this change to the baselineskip +% times : uses times font as the default +% linenumbers : turn on lineno package. +% trackchanges : required to see the revision mark up and print output +% letteredappendix: (was numbered appendix) Not needed because it is the default, will label appendix sections A, B, ... +% numberedappendix: Legacy command, will produce same results as lettered appendix, since we don't want more +% than one `section 1' in article: will cause problems for cross referencing. + +% anonymous: to not list authors/affiliations be listed + +\newif\ifmanu +\newif\iftwelvepoint +\newif\ifmodern +\newif\ifdoublespace +\newif\if@two@col +\newif\ifonecolstyle +\newif\iftwocolstyle + +\newif\ifrnaas +%% makes modern the style for rnaas +\DeclareOption{RNAAS}{\global\rnaastrue} +\DeclareOption{rnaas}{\global\rnaastrue} + + \DeclareOption{manuscript}{\twelvepointtrue\@two@colfalse\doublespacetrue\manutrue}% + +%% Preprints are like manuscript but are single spaced: +\newif\ifpreprint + \DeclareOption{preprint}{\@two@colfalse\preprinttrue\twelvepointtrue}% + +\newif\ifpreprinttwo + \DeclareOption{preprint2}{\@two@coltrue\preprinttwotrue\twelvepointtrue}% + + +%% New design suggested by +\DeclareOption{modern}{\@two@colfalse\twelvepointtrue\moderntrue} + +%% left in from older version, in case it could be useful: + + + +\DeclareOption{twocolumn}{\onecolstylefalse\twocolstyletrue\@two@coltrue\twelvepointfalse} + +%% default style +\DeclareOption{onecolumn}{\onecolstyletrue\twocolstylefalse} + +%% obsolete option +\DeclareOption{revtex4}{\typeout{=================^^J^^J!!! The revtex4 option no longer + allowed!^^J^^J Please download revtex4-1.cls^^J^^J + Thank-you!^^J^^J=================}\stop} + +\newif\if@two@col@app +\DeclareOption{twocolappendix}{\@two@col@apptrue} +\DeclareOption{onecolappendix}{\@two@col@appfalse}%% this is default + +\newif\iflongauthor +\DeclareOption{longauthor}{\global\longauthortrue} + +\newlength{\bibbaselineskip}\setlength{\bibbaselineskip}{3.075mm} + + \DeclareOption{astrosymb}{ + \def\astro#1{\leavevmode\hbox{\astro@font#1}}% + \def\load@astro@font{% +\iftwelvepoint + \font\astro@font=astrosym at 8pt +\else + \font\astro@font=astrosym at 7pt +\fi +}% + \AtBeginDocument{\load@astro@font} + } + +%% Default definition for \astro, in case astrosymb option has not +%% been used: +\def\astro#1{\typeout{^^J^^J Please use class option `astrosymb' to +access fonts for the \string\astro\space command +^^J^^J +}\stop} + + \def\apjsecfont{\normalsize} + \def\secnum@size{\small} + \def\subsecnum@size{\normalsize} + + \def\AppendixApjSectionMarkInTitle#1{\relax} +\newif\ifletteredappendix + \DeclareOption{letteredappendix}{\global\letteredappendixtrue + \def\AppendixApjSectionMarkInTitle#1{#1.\ } + } + +%% this option is obsolete, since letteredappendix is a more logical name; +%% but keeping it here in case someone uses it, set to be the same as +%% letteredappendix. + \DeclareOption{numberedappendix}{\global\letteredappendixtrue + \def\AppendixApjSectionMarkInTitle#1{#1.\ } + } + + \newif\if@number@appendix@floats\@number@appendix@floatsfalse + \DeclareOption{appendixfloats}{ + \@number@appendix@floatstrue + } + +%%%%%%%%%%%%% +%% AH + +%% This option changes the baselineskips in the definitions of \normalsize etc +%% to make them a bit smaller. +\newif\iftighten +\DeclareOption{tighten}{\global\tightentrue} + +%% AH +\newif\iftimes +\DeclareOption{times}{\global\timestrue} + +\newif\ifnumlines +\DeclareOption{linenumbers}{\global\numlinestrue} + +\newif\iftrack +\DeclareOption{trackchanges}{\global\tracktrue} + +\newif\ifanonymous +\DeclareOption{anonymous}{\global\anonymoustrue} + + +%% End AH Options + +\ExecuteOptions{onecolumn,onecolappendix,letteredappendix}% + +\ProcessOptions + +%%%%%%%%%%%%% +% + + \iftimes +%% Might be better to use apjfonts, from Alexey Vikhlinin's website +%% http://hea-www.harvard.edu/~alexey/emulateapj/apjfonts.sty +%%\usepackage{apjfonts} +%% but times.sty is ubiquitous, and many people may not have apjfonts.sty +%% or the fonts that it calls. +%% default fonts: +\usepackage{times} + \fi + +%%%%%%%%%%%%% + + \IfFileExists{revtex4-1.cls}{ + \def\@revtex@cls{revtex4-1} + }{ +\typeout{^^J^^J Please update your system to include +revtex4-1.cls^^J^^J}\stop + } +\def\@revtex@cls{revtex4-1} +\let\@startsection@from@latex=\@startsection + + +%% Passing options to revtex while loading: + \iftwelvepoint + \iflongauthor + \LoadClass[nofootinbib,showkeys,twoside,floatfix,unsortedaddress,flushbottom,12pt,aps,pra] + {\@revtex@cls} + \else + \LoadClass[nofootinbib,showkeys,twoside,floatfix,superscriptaddress,flushbottom,12pt,aps,pra] + {\@revtex@cls} + \fi + \else %not twelvepoint + \iflongauthor + \LoadClass[nofootinbib,showkeys,twoside,floatfix,unsortedaddress,flushbottom,10pt,aps,pra] + {\@revtex@cls} + \else + \LoadClass[nofootinbib,showkeys,twoside,floatfix,superscriptaddress,flushbottom,10pt,aps,pra] + {\@revtex@cls} + \fi + \fi + +%%%%%%%%%%%%%%%%%%%% + +\def\blankaffiliation{~}% + +%% needed? + \def\@eapj@cap@font{\bfseries} + \def\@eapj@figname{Figure} + \def\@eapj@tabname{Table} + +% Restore natbib package without sorting. +\def\NAT@sort{0} +\def\NAT@cmprs{0} + +% only redefine sort@cites for natbib versions < 2009 +\@ifundefined{NAT@sort@cites@}{\def\NAT@sort@cites#1{\edef\NAT@cite@list{#1}}}% + +\RequirePackage{latexsym}% +\RequirePackage{graphicx}% +\RequirePackage{amssymb}% + +\newcommand{\bibstyle@aas}{\bibpunct{(}{)}{;}{a}{}{,}}% +\@citestyle{aas}% + +\let\@startsection=\@startsection@from@latex +\def\baselinestretch{1.0} + +%% Default vertical space between horizontal lines. Can change definition +%% of arraystretch in the body of the paper; either for full article or +%% for a single table. +\AtBeginDocument{\def\arraystretch{1}} + +%% needed? +\def\raggedcolumn@sw#1#2{#2} % implement flushbottom as it was in revtex4 + +\RequirePackage{epsf,graphicx} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Font families +%% modification of bk10.clo, and bk12.clo, standard LaTeX distribution +%% +%% Implements doublespace used in `manuscript' option +%% Implements `tighten' option: make baselineskip smaller if `tighten' is used +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%% tighten only works with two column styles: +\iftwocolstyle\else\global\tightenfalse\fi + +%%% preprint, preprint2, manuscript are 12pt +%% Modified bk12.clo +\iftwelvepoint + +\renewcommand\normalsize{% +\ifdoublespace % manuscript + \iftighten + \@setfontsize\normalsize\@xiipt{20}% + \else + \@setfontsize\normalsize\@xiipt{24}% + \fi +\else + \iftighten + \@setfontsize\normalsize\@xiipt{13}% + \else + \ifmodern + \@setfontsize\normalsize\@xiipt{16}% + \else + \@setfontsize\normalsize\@xiipt{15}% + \fi + \fi +\fi %% end doublespace/no double space + \abovedisplayskip 12\p@ \@plus3\p@ \@minus7\p@ + \abovedisplayshortskip \z@ \@plus3\p@ + \belowdisplayshortskip 6.5\p@ \@plus3.5\p@ \@minus3\p@ + \belowdisplayskip \abovedisplayskip + \let\@listi\@listI} + +\normalsize + +\renewcommand\small{% +\ifdoublespace % manuscript + \@setfontsize\small\@xipt{20}% +\else +\ifmodern + \@setfontsize\small\@xipt{12}% +\else + \@setfontsize\small\@xipt{13.6}% +\fi\fi +%% end doublespace/no double space + \abovedisplayskip 11\p@ \@plus3\p@ \@minus6\p@ + \abovedisplayshortskip \z@ \@plus3\p@ + \belowdisplayshortskip 6.5\p@ \@plus3.5\p@ \@minus3\p@ + \def\@listi{\leftmargin\leftmargini + \topsep 9\p@ \@plus3\p@ \@minus5\p@ + \parsep 4.5\p@ \@plus2\p@ \@minus\p@ + \itemsep \parsep}% + \belowdisplayskip \abovedisplayskip +} + +\renewcommand\footnotesize{% +\ifdoublespace % manuscriptstyle + \@setfontsize\footnotesize\@xpt{18} +\else + \ifmodern + \@setfontsize\footnotesize\@xpt{11}% + \else + \@setfontsize\footnotesize\@xpt\@xiipt +\fi\fi + \abovedisplayskip 10\p@ \@plus2\p@ \@minus5\p@ + \abovedisplayshortskip \z@ \@plus3\p@ + \belowdisplayshortskip 6\p@ \@plus3\p@ \@minus3\p@ + \def\@listi{\leftmargin\leftmargini + \topsep 6\p@ \@plus2\p@ \@minus2\p@ + \parsep 3\p@ \@plus2\p@ \@minus\p@ + \itemsep \parsep}% + \belowdisplayskip \abovedisplayskip +} +\ifdoublespace % manuscript style +\renewcommand\scriptsize{\@setfontsize\scriptsize\@viiipt{14}} +\renewcommand\tiny{\@setfontsize\tiny\@vipt{10}} +\renewcommand\large{\@setfontsize\large\@xivpt{18}} +\renewcommand\Large{\@setfontsize\Large\@xviipt{22}} +\renewcommand\LARGE{\@setfontsize\LARGE\@xxpt{25}} +\renewcommand\huge{\@setfontsize\huge\@xxvpt{30}} +\else +\renewcommand\scriptsize{\@setfontsize\scriptsize\@viiipt{9.5}} +\renewcommand\tiny{\@setfontsize\tiny\@vipt\@viipt} +\renewcommand\large{\@setfontsize\large\@xivpt{22}} +\renewcommand\Large{\@setfontsize\Large\@xviipt{24}} +\renewcommand\LARGE{\@setfontsize\LARGE\@xxpt{28}} +\renewcommand\huge{\@setfontsize\huge\@xxvpt{30}} +\fi +\let\Huge=\huge +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +\else %% not twelvepoint, now tenpoint +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% no doublespace here, because the only doublespace is in `manuscript style' which is 12pt + +\renewcommand\normalsize{% +\iftighten + \@setfontsize\normalsize\@xpt{11.5}% +\else + \@setfontsize\normalsize\@xpt{12.5}% +\fi + \abovedisplayskip 10\p@ \@plus2\p@ \@minus5\p@ + \abovedisplayshortskip \z@ \@plus3\p@ + \belowdisplayshortskip 6\p@ \@plus3\p@ \@minus3\p@ + \belowdisplayskip \abovedisplayskip + \let\@listi\@listI} + +\normalsize + +\renewcommand\small{% +\iftighten + \@setfontsize\small\@ixpt{12}% +\else + \@setfontsize\small\@ixpt{11}% +\fi + \abovedisplayskip 8.5\p@ \@plus3\p@ \@minus4\p@ + \abovedisplayshortskip \z@ \@plus2\p@ + \belowdisplayshortskip 4\p@ \@plus2\p@ \@minus2\p@ + \def\@listi{\leftmargin\leftmargini + \topsep 4\p@ \@plus2\p@ \@minus2\p@ + \parsep 2\p@ \@plus\p@ \@minus\p@ + \itemsep \parsep}% + \belowdisplayskip \abovedisplayskip +} + +\renewcommand\footnotesize{% +\iftighten + \@setfontsize\footnotesize\@viiipt{9}% +\else + \@setfontsize\footnotesize\@viiipt{9.5}% standard eightpoint size +\fi + \abovedisplayskip 6\p@ \@plus2\p@ \@minus4\p@ + \abovedisplayshortskip \z@ \@plus\p@ + \belowdisplayshortskip 3\p@ \@plus\p@ \@minus2\p@ + \def\@listi{\leftmargin\leftmargini + \topsep 3\p@ \@plus\p@ \@minus\p@ + \parsep 2\p@ \@plus\p@ \@minus\p@ + \itemsep \parsep}% + \belowdisplayskip \abovedisplayskip +} + +%% Standard 10pt font sizes +\renewcommand\scriptsize{\@setfontsize\scriptsize\@viipt\@viiipt} +\renewcommand\tiny{\@setfontsize\tiny\@vpt\@vipt} +\renewcommand\large{\@setfontsize\large\@xiipt{14}} +\renewcommand\Large{\@setfontsize\Large\@xivpt{18}} +\renewcommand\LARGE{\@setfontsize\LARGE\@xviipt{22}} +\renewcommand\huge{\@setfontsize\huge\@xxpt{25}} +\renewcommand\Huge{\@setfontsize\Huge\@xxvpt{30}} + +\fi + +%% End font sizes +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + + +\setlength\smallskipamount{3\p@ \@plus 1\p@ \@minus 1\p@} +\setlength\medskipamount{6\p@ \@plus 2\p@ \@minus 2\p@} +\setlength\bigskipamount{12\p@ \@plus 4\p@ \@minus 4\p@} +\setlength\headheight{12\p@} +\def\@listi{\leftmargin\leftmargini + \parsep 4\p@ \@plus2\p@ \@minus\p@ + \topsep 8\p@ \@plus2\p@ \@minus4\p@ + \itemsep4\p@ \@plus2\p@ \@minus\p@} +\let\@listI\@listi +\@listi +\def\@listii {\leftmargin\leftmarginii + \labelwidth\leftmarginii + \advance\labelwidth-\labelsep + \topsep 4\p@ \@plus2\p@ \@minus\p@ + \parsep 2\p@ \@plus\p@ \@minus\p@ + \itemsep \parsep} +\def\@listiii{\leftmargin\leftmarginiii + \labelwidth\leftmarginiii + \advance\labelwidth-\labelsep + \topsep 2\p@ \@plus\p@\@minus\p@ + \parsep \z@ + \partopsep \p@ \@plus\z@ \@minus\p@ + \itemsep \topsep} +\def\@listiv {\leftmargin\leftmarginiv + \labelwidth\leftmarginiv + \advance\labelwidth-\labelsep} +\def\@listv {\leftmargin\leftmarginv + \labelwidth\leftmarginv + \advance\labelwidth-\labelsep} +\def\@listvi {\leftmargin\leftmarginvi + \labelwidth\leftmarginvi + \advance\labelwidth-\labelsep} + +% **************************************************** +% * TWO AND SINGLE ONE COLUMN STYLES: AV * +% **************************************************** +% + +%%%%% include atbeginend.sty by AV: + +% Copy \begin and \end to \BeginEnvironment and \EndEnvironment +\let\BeginEnvironment=\begin +\let\EndEnvironment=\end +%% \ifundefined from TeXbook +\def\IfUnDef#1{\expandafter\ifx\csname#1\endcsname\relax} +% Null command needed to eat its argument +\def\NullCom#1{} +\def\begin#1{% +% if defined \BeforeBeg for this environment, execute it +\IfUnDef{BeforeBeg#1}\else\csname BeforeBeg#1\endcsname\fi% +\IfUnDef{AfterBeg#1}% This is done to skip the command for environments + % which can take arguments, like multicols; YOU MUST NOT + % USE \AfterBegin{...}{...} for such environments! + \let\SaveBegEnd=\BeginEnvironment% +\else + % Start this environment + \BeginEnvironment{#1}% + % and execute code after \begin{environment} + \csname AfterBeg#1\endcsname + \let\SaveBegEnd=\NullCom +\fi +\SaveBegEnd{#1} +} +\def\end#1{% +% execute code before \end{environment} +\IfUnDef{BeforeEnd#1}\else\csname BeforeEnd#1\endcsname\fi% +% close this environment +\EndEnvironment{#1} +% and execute code after \begin{environment} +\IfUnDef{AfterEnd#1}\else\csname AfterEnd#1\endcsname\fi% +} +\long\def\BeforeBegin#1#2{\expandafter\gdef\csname BeforeBeg#1\endcsname {#2}} +\long\def\BeforeEnd #1#2{\expandafter\gdef\csname BeforeEnd#1\endcsname {#2}} +\long\def\AfterBegin #1#2{\expandafter\gdef\csname AfterBeg#1\endcsname {#2}} +\long\def\AfterEnd #1#2{\expandafter\gdef\csname AfterEnd#1\endcsname{#2}} + +%%%% end of atbeginend.sty + +% **************************************** +% * PAGE LAYOUT * +% **************************************** + +% Page size, spacing parameters, etc. + +\textwidth=7.1in +\columnsep=0.3125in +\parindent=0.125in +\voffset=-20mm +\hoffset=-7.5mm + +\topmargin=0in +\headheight=.15in +\headsep=0.5in +\oddsidemargin=0in +\evensidemargin=0in +\parskip=0cm + +\tolerance=600 % 3x "normal" value; cuts down on overfull complaints + +%% AV,MM, to have 64 lines per column, with textheight 25cm: +\textheight=64\baselineskip +\textheight=\baselinestretch\textheight +\ifdim\textheight>25.2cm\textheight=25.0cm\fi + +%% so that the margin at the bottom of the page is about equal to margin at top. -- AH +\advance\textheight -54pt + +\topskip\baselineskip +\maxdepth\baselineskip + + + +\def\eqsecnum{ + \@newctr{equation}[section] + \def\theequation{\hbox{\normalsize\arabic{section}-\arabic{equation}}}} + +%% running heads: +\def\lefthead#1{\gdef\@versohead{#1}} \lefthead{\relax} +\def\righthead#1{\ifanonymous\gdef\@rectohead{Anonymous author(s)}\else\gdef\@rectohead{#1}\fi} \righthead{\relax} +\let\shorttitle\lefthead +\let\shortauthors\righthead + +\def\ps@apjheads{\let\@mkboth\markboth + \def\@evenfoot{} + \def\@evenhead{\lower9mm\hbox to\textwidth{% + \rm\thepage\hfill\textsc{\@rectohead}\hfill}}} + \def\@oddfoot{} + \def\@oddhead{\lower9mm\hbox to\textwidth{ + \hfil\rm\textsc{\@versohead}\hfil \rm\thepage}} + +\pagestyle{apjheads} + +\@twosidetrue + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% TITLE PAGE % +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%% October 2017, adding preprint number capability +\newcount\rptnum +\newcount\rptloopnum +\def\reportnum#1{\global\advance\rptnum by 1 +\expandafter\gdef\csname report\the\rptnum\endcsname{\hbox to +\textwidth{\hskip.75\textwidth\relax#1\relax\hfill}}} + +\long\def\frontmatter@title@above{ +\ifrnaas +\vspace*{-\headsep}\vspace*{\headheight} +\footnotesize +\noindent{\sc Draft version \today}\\[2pt] +{\footnotesize Typeset using \LaTeX\ {\bf RNAAS} style in AASTeX631} +\par\vspace*{-\baselineskip}\vspace*{0.625in} +\else +\vbox to 0pt{\vskip-48pt\normalsize\rptloopnum=0\loop +\global\advance\rptloopnum by 1 +\expandafter\ifx\csname report\the\rptloopnum\endcsname\relax +\else +\csname report\the\rptloopnum\endcsname +\vskip1pt +\repeat +\vss +} +\ifmodern +\vglue-18pt +{\footnotesize +\raggedright +{\sc Draft version \today}\\[2pt] +{\footnotesize +Typeset using \LaTeX\ {\bf modern} style in AASTeX631} +\vskip48pt +} +\else +%% +\ifpreprint +\vspace*{-\headsep}\vspace*{\headheight} +\footnotesize +\noindent{\sc Draft version \today}\\[2pt] +{\footnotesize Typeset using \LaTeX\ {\bf preprint} style in AASTeX631} +\par\vspace*{-\baselineskip}\vspace*{0.625in} +\else +%% +\ifpreprinttwo +\vspace*{-\headsep}\vspace*{\headheight} +\footnotesize +{\footnotesize\textsc{\@journalinfo}}\par +{\footnotesize Typeset using \LaTeX\ {\bf preprint2} style in +AASTeX631} +\par\vspace*{-\baselineskip}\vspace*{0.625in} +\else +%% +\iftwocolstyle +\vspace*{-\headsep}\vspace*{\headheight} +\footnotesize +{\footnotesize\textsc{\@journalinfo}}\par +{\footnotesize Typeset using \LaTeX\ {\bf twocolumn} style in +AASTeX631} +\par\vspace*{-\baselineskip}\vspace*{0.625in} +\else +\ifmanu +\vspace*{-\headsep}\vspace*{\headheight} +\footnotesize +\noindent\textsc{\@journalinfo}\\[-8pt] +{\footnotesize Typeset using \LaTeX\ {\bf manuscript} style in +AASTeX631} +\par\vspace*{-\baselineskip}\vspace*{0.625in} +\else +%% Default +\vspace*{-\headsep}\vspace*{\headheight} +\footnotesize +{\footnotesize\textsc{\@journalinfo}}\par +{\footnotesize Typeset using \LaTeX\ default style in AASTeX631}%% default style +\par\vspace*{-\baselineskip}\vspace*{0.625in} +\fi\fi\fi\fi\fi +%% +\fi %% ends test to see if rnaas option was used; if rnaas is true + %% none of this command will be activated. +}% + +\def\frontmatter@title@produce{% + \begingroup +\ifnumlines\nolinenumbers\fi + \frontmatter@title@above + \frontmatter@title@format + \@title +%% October 2017, was +12pt + \@ifx{\@title@aux\@title@aux@cleared}{}{% +\ifanonymous\else%% added may 20, 2020 + \expandafter\frontmatter@footnote\expandafter{\@title@aux}% +\fi + }% + \par +%% \class@warn{Unused short title ignored}% +\ifmodern +\vskip-42pt +\else +\ifmanu +\vskip-60pt +\else + \frontmatter@title@below +\fi +\fi + \endgroup +}% + +\newcount\fncount +\newcount\endfncount +\long\def\tempfootnote#1{\global\advance\fncount by 1\relax% +\expandafter\gdef\csname +footnote\the\fncount\endcsname{\if@two@col\hsize=.5\textwidth +\advance\hsize by -18pt +\fi\relax#1}} + +\def\tempfootnoteintitle#1{} + +\long\def\ltx@foottext#1#2{% + \begingroup +\expandafter\ltx@make@current@footnote\expandafter{\@mpfn}{#1}% +\@footnotetext{\vtop{\iftwocolstyle\hsize=.5\textwidth +\advance\hsize-18pt +\fi #2\vskip2pt}}% fixed for two col style, march 15, 2019 + \endgroup +}% + + +\def\kickoutfootnotes{\c@footnote=0\relax% +\loop\advance\endfncount by 1\relax% +\expandafter\ifx\csname footnote\the\endfncount\endcsname\relax% +\else% +\def\thempfn{\fnsymbol{footnote}}% +\advance\c@footnote by 1\relax% +\unskip\footnote{\csname footnote\the\endfncount\endcsname}% +\repeat} + +%% +\renewcommand\title[2][]{% +\def\@title{\setbox0=\vbox{\let\footnote\tempfootnote #2}% +{\let\footnote\tempfootnoteintitle%\uppercase +{#2}}%% right place for kickoutfootnotes below +\kickoutfootnotes +\ifdoublespace\vskip 3\baselineskip\fi +}% + \def\@shorttitle{#1}% + \let\@AF@join\@title@join +}% + +\def\frontmatter@title@format{ +%% No exception for rnaas, May, 2019 +%\ifrnaas +%\large\scshape\centering +%\else +\normalsize +%% added Mar 2019 +\bf\centering +%\fi +} + +\def\frontmatter@title@below{\vskip8pt}% + + +\def\frontmatter@authorformat{\small\advance\baselineskip-3pt +\parskip=0pt\ifrnaas\else\scshape\fi +\ifmodern +\vskip48pt +\centering +\leftskip=.05in plus 1fil +\rightskip=.05in plus 1 fil +\baselineskip=13pt +\else +\centering +\fi +}% + + +\def\frontmatter@affiliationfont{\normalfont\footnotesize +%% changed october 2017 +\it +\iflongauthor\else +\ifrnaas\else +\rightskip-12pt plus 1fil +\leftskip6pt \parindent-4pt +\fi\fi +}% + + \def\frontmatter@finalspace{\ifrnaas\vspace*{-\baselineskip}\vspace*{0.0in} +\else +\vskip-24pt\fi} + +\def\@separator{\\}% + +\newcounter{front@matter@foot@note}\setcounter{front@matter@foot@note}{0} + +\iflongauthor% +\renewcommand\affiliation[1]{% +\parskip=2pt +\def\@centercr{\vrule depth 3pt width0pt\vskip1sp} + \move@AU\move@AF% +\iflongauthor\let\@listand\relax\fi + \begingroup% + \@affiliation{%\hspace*{2mm} +\ifnum\countauthors<\AuthorCollaborationLimit + #1\ifmodern\iflongauthor\baselineskip=12pt\else\vskip2pt\fi\else\baselineskip=11pt +\fi\fi +\ifnum\countauthors=\AuthorCollaborationLimit + #1\ifmodern\iflongauthor\baselineskip=12pt\else\vskip2pt\fi\else\baselineskip=11pt +\fi\fi +\iflongauthor \vskip-10pt\ifnum\countauthors>\AuthorCollaborationLimit\iftwelvepoint\vskip-3pt\else\iftwocolstyle\else\vskip-6pt\fi\fi\fi% +\fi +}% +\let\@centercr\savecentercr}% +\else +%% older version +\renewcommand\affiliation[1]{% + \move@AU\move@AF% + \begingroup% + \@affiliation{%\hspace*{2mm} +%% october 2017 changes: +\centering + #1\ifmodern +\baselineskip=9.5pt + \else + \iftwelvepoint + \ifpreprint\baselineskip=12pt\else\ifpreprinttwo\else\baselineskip19pt\fi\fi\else \baselineskip=9.5pt\fi +\fi}% +}% +\fi %% end switch for longauthor + +% ABSTRACT +\def\frontmatter@abstractfont{\normalsize\parindent=9pt +}% +%% october 2017 +\def\frontmatter@abstractwidth{478pt} +\def\frontmatter@preabstractspace{12pt} +\def\frontmatter@postabstractspace{12pt} + +\def\abstractname{ABSTRACT} +\long\def\frontmatter@abstractheading{% + \begingroup + \centering +\ifmodern\else\hskip34pt \fi \abstractname + \vskip 1mm + \par + \endgroup +}% + +\newif\ifabstract% +\renewenvironment{frontmatter@abstract}{% + \aftermaketitle@chk{\begin{abstract}}% +\global\abstracttrue + \global\setbox\absbox\vbox\bgroup + \color@begingroup +%% width of abstract changed oct 2017 +\ifmodern + \columnwidth\textwidth + \hsize\columnwidth +\else +\hsize = 478pt +\fi + \@parboxrestore + \def\@mpfn{mpfootnote}\def\thempfn{\thempfootnote)}\c@mpfootnote\z@ % should be footnote, not mpfootnote? +% \let\@footnotetext\frontmatter@footnotetext + \minipagefootnote@init + \let\set@listindent\set@listindent@ + \let\@listdepth\@mplistdepth \@mplistdepth\z@ + \let@environment{description}{frontmatter@description}% + \@minipagerestore + \@setminipage + \frontmatter@abstractheading + \frontmatter@abstractfont +% \let\footnote\mini@note +\ifmodern\else\everypar={\leftskip=34pt}\fi +% \expandafter\everypar\expandafter{\the\everypar\addcontents@abstract\everypar{}}% +\ifnumlines\let\go\linenumbers\else\let\go\relax\fi\go +}{% +\ifnumlines\let\go\endlinenumbers\else\let\go\relax\fi\go + \par + \unskip + \minipagefootnote@here + \@minipagefalse %% added 24 May 89 + \color@endgroup +\egroup% end setbox\absbox +}% + +\let\abstract\frontmatter@abstract + +\def\frontmatter@abstract@produce{% + \par + \preprintsty@sw{% + \do@output@MVL{% + \vskip\frontmatter@preabstractspace + \vskip200\p@\@plus1fil + \penalty-200\relax + \vskip-200\p@\@plus-1fil + }% + }{% + \addvspace{\frontmatter@preabstractspace}% + }% + \begingroup + \dimen@\baselineskip + \setbox\z@\vtop{\unvcopy\absbox}% + \advance\dimen@-\ht\z@\advance\dimen@-\prevdepth + \@ifdim{\dimen@>\z@}{\vskip\dimen@}{}% + \endgroup + \begingroup + \prep@absbox +%% centered, oct 2017 +\unvbox\absbox + \post@absbox + \endgroup + \@ifx{\@empty\mini@notes}{}{\mini@notes\par}% + \addvspace\frontmatter@postabstractspace +\global\abstractfalse +\vskip12pt +}% + +\newif\ifbib + +% **************************************** +% * KEYWORDS * +% **************************************** + + + \def\@keys@name{\textit{Keywords:}\/~\mbox{}}% + +\newlength{\keys@width} +\def\frontmatter@keys@format{\ifmodern\vskip0pt\else\vspace*{0.5mm}\fi% + \settowidth{\keys@width}{\normalsize\@keys@name}% +\ifmodern\else +\rightskip=0.5in +\leftskip=34pt +\fi +\parindent=0pt% + \hangindent=\keys@width\hangafter=1\normalsize}% +\def\@keywords@produce#1{% + \showKEYS@sw{% + \begingroup% + \frontmatter@keys@format% + \@keys@name#1 +\vrule depth 12pt width 0pt +\ifnobreakafterkeywords +\vrule depth 24pt width0pt\fi +\par + \endgroup + }{% + \@if@empty{#1}{}{% + \class@warn{If you want your keywords to appear in your output, use document class option showkeys}% + }% + }% +}% + +\let\subjectheadings=\keywords + + +% **************************************** +% * FOOTNOTES * +% **************************************** + +%% legacy notes and footnote code + +% Footnotes on the last page: user issues \lastpagefootnotes. It catches all +% footnotes and issues them before \begin{refernces} or +% \begin{\thebibliography} or \begin{appendix}, whichever comes first, +% at the end of right column. +\newcounter{lastfootnote} +\let\orig@footnote=\footnote +% +\def\spit@out@footnotes@{\addtocounter{footnote}{-\c@lastfootnote}\vspace*{-\baselineskip}\vspace*{\skip\footins}\bgroup\footnotesize\lastfootnote\par\egroup\let\footnote=\orig@footnote} +% +\let\spit@out@footnotes\relax +% +\long\def\lastpagefootnotes{% +\raggedbottom% Have to use flushbottom with revtex4-1 but it eats away + % last page footnotes +\setcounter{lastfootnote}{0} +\long\gdef\lastfootnote{\mbox{}} +\let\spit@out@footnotes\spit@out@footnotes@ +\long\def\footnote##1{\refstepcounter{lastfootnote}\footnotemark\g@addto@macro\lastfootnote{\\[\footnotesep]\refstepcounter{footnote}\mbox{}\hspace*{3mm}\textsuperscript{\thefootnote}~##1}} +% We need to mess with footnotes in appendix only if it is in a +% different mode (twocol vs onecol) than the main text +\def\mess@with@appendix@footnotes{ +\BeforeBegin{appendix}{\spit@out@footnotes\let\spit@out@footnotes\relax} +\BeforeEnd{appendix}{\spit@out@footnotes\let\spit@out@footnotes\relax} +\AfterEnd{appendix}{\let\footnote=\orig@footnote} +} + +\if@two@col + \if@two@col@app\else + \mess@with@appendix@footnotes + \fi +\fi + +\BeforeBegin{references}{\spit@out@footnotes\let\spit@out@footnotes\relax} +\BeforeBegin{thebibliography}{\spit@out@footnotes\let\spit@out@footnotes\relax} +% in case \lastpagefootnotes were given inside \begin{appendix}\end{appendix}, +\AfterEnd{references}{\let\footnote=\orig@footnote} +\AfterEnd{thebibliography}{\let\footnote=\orig@footnote} +} +\let\lastpagefootnote=\lastpagefootnotes + +%% probably not needed: +\def\notetoeditor#1{}% % We do not need notes to editor in the preprint +\def\placetable#1{}% % We do not need notes to editor in the preprint +\def\placefigure#1{}% % We do not need notes to editor in the preprint + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +\ifdoublespace %used for manuscript +\footnotesep 12pt +\skip\footins 36pt +\else +\footnotesep 12pt +\skip\footins 24pt +\fi + +\let\footnoterule\relax + +\def\@makefntext#1{\hsize=\columnwidth\mbox{}\hspace*{3mm}\@makefnmark~#1} + + +% **************************************** +% * SECTIONS * +% **************************************** + +\setcounter{secnumdepth}{3} + +\newcount\tempsectnum + +\newif\if@firstsection \@firstsectiontrue + + +\def\section{% +\ifanonymous\nocollaboration{0}\fi +\if@firstsection +%% In case no collaboration is listed: +\ifcollaborationon\else\let\doauthor\olddoauthor +\ifanonymous \else +\let\allauthors=\oldallauthors\fi +\fi +%\edef\currauthorlimit{\the\AuthorCollaborationLimit} +%\collaboration{\currauthorlimit}{} + \maketitle +\global\@firstsectionfalse + \setcounter{footnote}{\thefront@matter@foot@note}% + \let\footnotetext=\old@foot@note@text + \let\footnotemark=\old@foot@note@mark +\ifnobreakafterkeywords +\ifmodern\vskip24pt +\else +\vskip12pt\fi%% +\goodbreak +\else +\ifrnaas\else + \clearpage\fi +\fi + \if@two@col + \twocolumngrid + \fi +\fi +\tempsectnum=\the\c@section +\advance\tempsectnum by 1 +\xdef\cref@currentlabel{section \the\tempsectnum} + \@startsection{section}{1}{\z@}{9pt plus 1pt minus + 1pt}{4pt}{\apjsecfont\center}} + +\def\subsection{\@startsection{subsection}{2}{\z@}{9pt plus 1pt minus 1pt}{4pt}% + {\normalsize\itshape \center}} + +\def\subsubsection{\@startsection{subsubsection}{3}{\z@}% + {2ex plus 1ex minus .2ex}{1ex plus .2ex}{\small\itshape \center}} + +\def\paragraph{\@startsection{paragraph}{4}{\z@}% + {1.5ex plus 1ex minus .2ex}{0pt}{\small\itshape}} + +\def\subparagraph{\@startsection{subparagraph}{5}{\z@}% + {1ex plus 1ex minus .2ex}{-0.5\parindent}{\small\itshape}} + + +\def\thesection{\arabic{section}} +\def\thesubsection{\thesection.\arabic{subsection}} +\def\thesubsubsection{\thesubsection.\arabic{subsubsection}} +\def\theparagraph{\thesubsubsection.\arabic{paragraph}} +\def\p@section {} +\def\p@subsection {} +\def\p@subsubsection {} +\def\p@paragraph {} +\def\p@subparagraph {} + + +\def\sec@upcase#1{\uppercase{#1}} +\def\subsec@upcase#1{\relax{#1}} + +% +% How the section number will appear in the section title - AV +\def\ApjSectionMarkInTitle#1{\ifrnaas\else #1.\ \fi} +\def\ApjSectionpenalty{0} + + +\def\@sect#1#2#3#4#5#6[#7]#8% +{\ifnum#2=1\setbox0=\hbox{\def\label##1{\gdef\templabel{##1}}#7}\fi +\@tempskipa #5\relax + \ifdim \@tempskipa >\z@ \begingroup + #6\relax + \ifnum #2>\c@secnumdepth \def \@svsec {}\else + \refstepcounter{#1} \edef \@svsec {\ApjSectionMarkInTitle + {\csname the#1\endcsname}}\fi + \@hangfrom {\hskip #3\relax + \ifnum #2=1{\secnum@size {\rm\@svsec~}}% + \else {\subsecnum@size {\rm\@svsec~}}\fi }% + {\interlinepenalty \@M + \ifnum #2=1\sec@upcase{#8}% + \else \subsec@upcase{#8}\fi\par}\endgroup + \csname #1mark\endcsname {#7}\addcontentsline{toc}{#1}% + {\ifnum #2>\c@secnumdepth \else \protect \numberline + {\csname the#1\endcsname }\fi #7}% + \else + \ifnum #2>\c@secnumdepth \def \@svsec {}\else + \refstepcounter{#1} \edef \@svsec {\ApjSectionMarkInTitle + {\csname the#1\endcsname}}\fi + \def \@svsechd {#6\hskip #3% + \ifnum #2=1{\secnum@size{\rm\@svsec~}}\else{\subsecnum@size{\rm\@svsec~}}\fi% + \ifnum #2=1\sec@upcase{#8}\else\subsec@upcase{#8}\fi% + \ifnum #2=4\hskip 0.4ex{\rm ---}\fi% + \csname #1mark\endcsname {#7}\addcontentsline{toc}{#1}% + {\ifnum #2>\c@secnumdepth \else \protect \numberline {\csname + the#1\endcsname }\fi #7}}\fi \@xsect {#5} \penalty \ApjSectionpenalty +%-refstepcounter is now within a group. So \@currentlabel, which is normally +%-set by \refstepcounter is hidden within a group. Need to set it manually. +\protected@edef\@currentlabel{\csname p@#1\endcsname\csname +the#1\endcsname} +\expandafter\ifx\csname templabel\endcsname\relax +\let\go\relax +\else +\def\go{\label{\templabel}}\fi\go +\let\templabel\relax +} + +\def\@ssect#1#2#3#4#5{\@tempskipa #3\relax + \ifdim \@tempskipa>\z@ + \begingroup #4\@hangfrom{\hskip #1}{\interlinepenalty \@M + \sec@upcase{#5}\par}\endgroup + \else \def\@svsechd{#4\hskip #1\relax \sec@upcase{#5}}\fi + \@xsect{#3} +% MM: +\penalty \ApjSectionpenalty} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% changed to begin...end form, May 20,2020, AH +%% Acknowledgments, use \begin{acknowledgments}...\end{acknowledgments} +%% or \begin{acknowledgements}...\end{acknowledgements} + +{\catcode`#=12 +\gdef\hashmark{#}} + +\def\xacknowledgments{acknowledgments} +\def\xacknowledgements{acknowledgements} +\newbox\ackbox + +\def\acknowledgments{% +\ifx\@currenvir\xacknowledgments\let\go\relax\else +\let\go\stop +\typeout{x^^J^^J^^J^^J^^J^^J^^J^^J + ===================^^J +In AASTeX v6.3.1 the \string\acknowledgments\space command has been deprecated.^^J^^J +Instead, please use the begin/end form:^^J^^J +"\string\begin\string{acknowledgments\string}...\string\end\string{acknowledgments\string}"^^J^^J +when using acknowledgments.^^J^^J See here: +\url{https://journals.aas.org/aastexguide/\hashmark acknowledgments} +^^J^^J + for more +details.^^J + ===================^^J +}% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Printed error +\vskip12pt +\hrule height 1pt +\vskip12pt +\noindent ERROR: +In AASTeX v6.3.1 the {\tt\string\acknowledgments} command has been +deprecated.\\ +Instead, please use the begin/end form:\\ +{\tt +\string\begin\string{acknowledgments\string}...\string\end\string{acknowledgments\string}}\\ +when using acknowledgments. For more details, see:\\ +\url{https://journals.aas.org/aastexguide/\hashmark acknowledgments} +% +\fi\go +%% +\global\setbox\ackbox=\vbox\bgroup +\expandafter\ifx\csname internallinenumbers\endcsname\relax\else +\begin{internallinenumbers} +\fi +\vskip 5.8mm plus 1mm minus 1mm +\vskip1sp +%\section*{Acknowledgments} +\noindent\ignorespaces} + +\def\endacknowledgments{ +\expandafter\ifx\csname internallinenumbers\endcsname\relax\else +\end{internallinenumbers} +\fi +\egroup%% completes ackbox +\ifanonymous +\vskip 5.8mm plus 1mm minus 1mm +\vskip1sp +%\section*{Acknowledgments} +\centerline{(Acknowledgments anonymized for review)} +\else +\vbox{\unvbox\ackbox} +\fi\vskip6pt} + +%% alternate spelling +\def\acknowledgements{% +\ifx\@currenvir\xacknowledgements\let\go\relax\else +\let\go\stop +\typeout{x^^J^^J^^J^^J^^J^^J^^J^^J + ===================^^J +In AASTeX v6.3.1 the \string\acknowledgements\space command has been deprecated.^^J^^J +Please use the begin/end form:^^J^^J +"\string\begin\string{acknowledgements\string}...\string\end\string{acknowledgements\string}"^^J^^J +when using acknowledgements.^^J^^J See here: +\href{https://journals.aas.org/aastexguide/\hashmark acknowledgments} +{https://journals.aas.org/aastexguide/\hashmark acknowledgments} +^^J^^J + for more +details.^^J + ===================^^J +}% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Printed error +\vskip12pt +\hrule height 1pt +\vskip12pt +\noindent ERROR: +In AASTeX v6.3.1 the {\tt\string\acknowledgements} command has been +deprecated.\\ +Instead, please use the begin/end form:\\ +{\tt +\string\begin\string{acknowledgements\string}...\string\end\string{acknowledgements\string}}\\ +For more details, see:\\ +\url{https://journals.aas.org/aastexguide/\hashmark acknowledgments} +% +\fi\go +%% +\global\setbox\ackbox=\vbox\bgroup +\expandafter\ifx\csname internallinenumbers\endcsname\relax\else +\begin{internallinenumbers} +\fi +\vskip 5.8mm plus 1mm minus 1mm +\vskip1sp +%\section*{Acknowledgments} +\noindent\ignorespaces} + +\def\endacknowledgements{ +\expandafter\ifx\csname internallinenumbers\endcsname\relax\else +\end{internallinenumbers} +\fi +\egroup%% completes ackbox +\ifanonymous +\vskip 5.8mm plus 1mm minus 1mm +\vskip1sp +%\section*{Acknowledgements} +\centerline{(Acknowledgements anonymized for review)} +\else +\vbox{\unvbox\ackbox} +\fi\vskip6pt} + + + + + + +% **************************************** +% * APPENDIX * +% **************************************** + +\newcounter{remember@figure@num} +\newcounter{remember@table@num} + +% this was an environment earlier, which doesn't make sense since we don't +% do \begin{appendix}...\end{appendix}. Changed to \appendix which is how it is used. + +% numberedappendix: Needed to label appendix sections A, B, . +% appendixfloats: Needed. ?? + +\newif\ifappendixon +\def\appendix{\global\appendixontrue +\if@two@col +\onecolumngrid +\noindent\mbox{}\vrule height 24pt width0pt\hfill{\apjsecfont APPENDIX}\hfill\mbox{}\par +\vskip18pt + \if@two@col@app\global\@two@coltrue\twocolumngrid \fi + % above, we want onecolumngrid to be default. Only twocolumn is asked for in documentclass option +\else +\noindent\mbox{}\vrule height 24pt width0pt\hfill{\apjsecfont +APPENDIX}\hfill\mbox{}\par +\vskip18pt + \if@two@col@app\global\@two@coltrue\twocolumngrid + \fi\fi +% \vrule used for extra space; otherwise revtex4-1 sometimes eats +% away the last line before appendix + \nopagebreak\medskip\@nobreaktrue\def\ApjSectionpenalty{\@M} + \@firstsectionfalse + \setcounter{section}{0} + \setcounter{subsection}{0} + \setcounter{equation}{0} +%% +\ifletteredappendix + \def\thesection{\Alph{section}} + \def\theequation{\hbox{\Alph{section}\arabic{equation}}} +%% these are NOT supposed to reset to zero +%\setcounter{table}{0} +%\setcounter{figure}{0} +\fi +%% +\if@number@appendix@floats +% we don't want to set equations to zero in appendix, because there +% might then be two equation 1's, etc., confusing for cross referencing. +%\setcounter{equation}{0} + \def\thesection{\Alph{section}} + \def\theequation{\hbox{\Alph{section}\arabic{equation}}} + \def\section{\@startsection {section}{1}{\z@} + {10pt}{5pt}{\centering\scshape\apjsecfont}} +\else +% Do not use appendix numbers in the titles + \def\ApjSectionMarkInTitle{\AppendixApjSectionMarkInTitle} +\fi +\ifappletter +\let\savesection\section +\def\section{\resetapptablenumbers\savesection} +\fi +} +% + + +%% + +% **************************************** +% * BIBLIOGRAPHY * +% **************************************** + +\renewenvironment{references}[0]{ + \onecolumngrid + \par + \vspace{10pt plus 3pt} + \noindent \makebox[\textwidth][c]{\small\scshape REFERENCES} + \par + \vspace*{4pt plus 3pt} + \set@column@hsize{2}\twocolumngrid +%% Jan29, 2021, added \ifonecolstyle, \ifpreprinttwo +\ifnumlines +\ifonecolstyle +\ifpreprinttwo\else +\advance\linenumbersep-12pt\fi\fi\fi + \parindent=0cm \parskip=0cm + \def\baselinestretch{1.0} + \footnotesize \baselineskip=\baselinestretch\bibbaselineskip plus 1pt + minus 1pt \interlinepenalty \@M + \hyphenpenalty=10000 + \frenchspacing % AV - to get right spacing after ``et al.'' + \def\refpar{\par\hangindent=1.2em\hangafter=1}} +{ + \onecolumngrid +} + +% redefine thebibliography + +% remove numbers from the reference list +\def\@biblabel#1{\relax} + +\newskip\bibskip +\bibskip=0pt plus 1pt +\let\savebibitem\bibitem +\def\bibitem{\vskip\bibskip\savebibitem} +\newdimen\bibindent +\renewenvironment{thebibliography}[1]{\global\bibtrue +%%\ifrnaas\newpage\fi% Not wanted, March 2019 +\onecolumngrid +\vspace{20pt} +\goodbreak + \hbox to\textwidth{\hss\normalsize REFERENCES\hss} +\vspace{6pt}\parskip=0pt +\twocolumngrid +%% Jan29, 2021, added \ifonecolstyle +\ifnumlines +\ifonecolstyle +\ifpreprinttwo\else +\advance\linenumbersep-12pt\fi\fi\fi +\par + \raggedright +\small +\ifmodern\else + \vspace{10pt plus 3pt}\fi +\par +\topsep=0pt + \list{}% + { + \parindent=0pt \parskip=1pt plus 1pt \parsep=0pt % AV + \bibindent=0pt % +\ifmodern\vskip-12pt +\baselineskip=13pt plus 1pt +\else +\ifdoublespace +\baselineskip=20pt +\else +\baselineskip=13pt plus 1pt \fi\fi \interlinepenalty \@M % AV + \frenchspacing % AV - to get right spacing after ``et al.'' + \hyphenpenalty=10000 + \itemindent=-1.0em % + \itemsep=0pt % + \listparindent=0pt % + \settowidth\labelwidth{0pt} % + \labelsep=0pt % + \leftmargin=1.0em + \advance\leftmargin\labelsep +%%% \usecounter{enumiv}% + \let\p@enumiv\@empty + \renewcommand\theenumiv{\relax}}% + \sloppy\clubpenalty10000\widowpenalty10000% + \sfcode`\.\@m\relax +%%%\item[] This May be necessary, but causes extra vertical space in first column +%%% of the bibliography. +} + {\def\@noitemerr + {\@latex@warning{Empty `thebibliography' environment}}% +\endlist + \onecolumngrid % to balance references +\global\bibfalse +\newpage + } + +% %% AV: + +\def\reference{\@ifnextchar\bgroup {\@reference} + {\@latexerr{Missing key on reference command} + {Each reference command should have a key corresponding to a markcite somewhere in the text}}} +\def\@reference#1{\refpar} + +%% subtitle header and journal info, legacy, probably not needed +% \def\submitted#1{\gdef\@submitted{#1}} +% \let\slugcomment\submitted % slugcomment == submitted +% \submitted{Draft version \today} +% \journalinfo{\@submitted} + + \def\journalinfo#1{\gdef\@journalinfo{#1}} + \journalinfo{Draft version \today} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% Equations % +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +% EQNARRAY with reduced spacing around tab characters - AV +\def\eqnarray{% + \stepcounter{equation}% + \def\@currentlabel{\p@equation\theequation}% + \global\@eqnswtrue + \setlength{\arraycolsep}{0.25\arraycolsep} + \m@th + \global\@eqcnt\z@ + \tabskip\@centering + \let\\\@eqncr + $$\everycr{}\halign to\displaywidth\bgroup + \hskip\@centering$\displaystyle\tabskip\z@skip{##}$\@eqnsel + &\global\@eqcnt\@ne\hskip \tw@\arraycolsep \hfil${##}$\hfil + &\global\@eqcnt\tw@ \hskip \tw@\arraycolsep + $\displaystyle{##}$\hfil\tabskip\@centering + &\global\@eqcnt\thr@@ \hb@xt@\z@\bgroup\hss##\egroup + \tabskip\z@skip + \cr + } + +% **************************************** +% * TABLES AND FIGURES * +% **************************************** + +\def\@arstrut@hline@clnc{0.5\p@}% % Klootch: magic number + +\setcounter{topnumber}{7} + +\setlength{\belowcaptionskip}{4pt}% +\setlength{\abovecaptionskip}{5pt} + +\setlength{\textfloatsep}{9pt} +\setlength{\dbltextfloatsep}{0pt} + +% \addtolength{\textfloatsep}{17mm plus 10mm minus 10mm} + % \addtolength{\dbltextfloatsep}{7mm plus 10mm minus 10mm} + + +\renewcommand{\topfraction}{1.0} +\renewcommand{\bottomfraction}{1.0} +\renewcommand{\textfraction}{0.0} +\renewcommand{\dbltopfraction}{0.85} +\renewcommand{\dblfloatpagefraction}{0.85} +\setcounter{topnumber}{9} +\setcounter{bottomnumber}{9} +\setcounter{totalnumber}{20} +\setcounter{dbltopnumber}{9} + +% Copied from revtex4.cls; without it, captions are centered +\def\@xfloat@prep{% + \let\footnote\footnote@latex + \def\@mpfn{mpfootnote}% + \def\thempfn{\thempfootnote}% + \c@mpfootnote\z@ + \let\@footnotetext\@mpfootnotetext + \let\H@@footnotetext\@mpfootnotetext + \let\@makefntext\@mpmakefntext +}% + + +%%%%%%%%%%%% \cutinhead + +%% Number of \pt@ncol set when \tablecolumns{} used at beginning of +%% deluxetable. + +\def\@ptabularcr{\\} +\newcommand\cutinhead[1]{% + \noalign{\vskip 1.5ex}% + \hline + \@ptabularcr + \noalign{\vskip -1.5ex}% + \multicolumn{\pt@ncol}{c}{#1}% + \@ptabularcr + \noalign{\vskip .8ex}% + \hline + \@ptabularcr + \noalign{\vskip -2ex}% +}% + +\newcommand\sidehead[1]{% + \noalign{\vskip 1.5ex}% +% \hline +% \@ptabularcr +% \noalign{\vskip -1.5ex}% + \multicolumn{\pt@ncol}{l}{#1}% + \@ptabularcr + \noalign{\vskip .8ex}% +% \hline +% \@ptabularcr +% \noalign{\vskip -2ex}% +}% + + +%% these don't seem to be relevant: +\newcommand\figcaption{\@testopt{\@xfigcaption}{}}% +%% suggested by Joern Wilms +\def\@figcaption#1{{\def\@captype{figure}\caption{\footnotesize #1}}} +\def\@xfigcaption[#1]#2{{\def\@captype{figure}\caption{\footnotesize +#2}}} + +\def\thefigure{\@arabic\c@figure} + +\def\fnum@figure{{\footnotesize{\@eapj@cap@font\rm +\mbox{\@eapj@figname~\thefigure}% <== was period here +}}} + +\def\thetable{\@arabic\c@table} +%%% Table captions without making a floating table +\def\tabcaption{\@ifnextchar[{\@xtabcaption}{\@tabcaption}} +\def\@tabcaption#1{{\def\@captype{table}\caption{#1}}} +\def\@xtabcaption[#1]#2{{\def\@captype{table}\caption{#2}}} + +%% redefined below +\def\fnum@table{{\@eapj@cap@font \@eapj@tabname~\thetable}} + + \let\fnum@ptable=\fnum@table + \def\fnum@ptablecont{{\centering{\scshape Table~\thetable}---{\itshape + Continued}}}% + \long\def\@make@caption@text#1#2{% + {\small\centering#1{\scshape #2}\par\vskip1.4ex} + }% + +\long\def\@makecaption@plano@cont#1#2{% + {\small \centering#1\par}\vskip1.4ex\relax +}% + + +%% Commands from aastex.cls: + +% This has been redefined below +%\newcommand\dataset{\@testopt\@dataset{[}}% +%\def\@dataset[#1]#2{#2}% + +\newcommand\facility{\@testopt\@facility{[}}% +\def\@facility[#1]#2{{\vskip6pt{\large\it Facility:} #2}}% + +\newcommand\facilities{\@testopt\@facilities{[}}% +\def\@facilities[#1]#2{{\vskip6pt{\large\it Facilities:} #2}}% + + +\long\def\software{\bgroup\@testopt \@software {[}} +\def\@software[#1]#2{\vskip 6pt{ +\frenchspacing +\iftwelvepoint +\font\foo=cmr12 +\else +\font\foo=cmr10\fi +%% +\fontdimen2\foo=3pt %% Changed from 1.5pt to 3pt, March12, 2019 +%% +{\large \it Software: } +#2 +%% returning to original fontdimen +\iftwelvepoint +\fontdimen2\foo=3.91663pt +\else +\fontdimen2\foo=3.33333pt +\fi +}\egroup} + + + + + +\newcommand\object{\@testopt\@object{[}}% +\def\@object[#1]#2{#2}% +\newcommand\objectname{\@testopt\@objectname{[]}}% +\def\@objectname[#1]#2{#2}% +\newlength{\plot@width} +\def\eps@scaling{1.0}% +\newcommand\epsscale[1]{\def\eps@scaling{#1}}% +\newcommand\plotone[1]{% + \centering + \leavevmode + \setlength{\plot@width}{0.85\linewidth} + \includegraphics[width={\eps@scaling\plot@width}]{#1}% +}% +\newcommand\plottwo[2]{% + \centering + \leavevmode + \setlength{\plot@width}{0.425\linewidth} + \includegraphics[width={\eps@scaling\plot@width}]{#1}% + \hfil + \includegraphics[width={\eps@scaling\plot@width}]{#2}% +}% +\newcommand\plotfiddle[7]{% + \centering + \leavevmode + \vbox\@to#2{\rule{\z@}{#2}}% + \includegraphics[% + scale=#4, + angle=#3, + origin=c + ]{#1}% +}% +\newcommand\figurenum[1]{% + \def\thefigure{#1}% + \let\@currentlabel\thefigure + \addtocounter{figure}{\m@ne}% +}% + +\newcommand\phn{\phantom{0}}% +\newcommand\phd{\phantom{.}}% +\newcommand\phs{\phantom{$-$}}% +\newcommand\phm[1]{\phantom{#1}}% +\let\la=\lesssim % For Springer A&A compliance... +\let\ga=\gtrsim +\newcommand\sq{\mbox{\rlap{$\sqcap$}$\sqcup$}}% +\newcommand\arcdeg{\mbox{$^\circ$}}% +\newcommand\arcmin{\mbox{$^\prime$}}% +\newcommand\arcsec{\mbox{$^{\prime\prime}$}}% +\newcommand\fd{\mbox{$.\!\!^{\mathrm d}$}}% +\newcommand\fh{\mbox{$.\!\!^{\mathrm h}$}}% +\newcommand\fm{\mbox{$.\!\!^{\mathrm m}$}}% +\newcommand\fs{\mbox{$.\!\!^{\mathrm s}$}}% +\newcommand\fdg{\mbox{$.\!\!^\circ$}}% +\newcommand\farcm@mss{\mbox{$.\mkern-4mu^\prime$}}% +\let\farcm\farcm@mss +\newcommand\farcs@mss{\mbox{$.\!\!^{\prime\prime}$}}% +\let\farcs\farcs@mss +\newcommand\fp{\mbox{$.\!\!^{\scriptscriptstyle\mathrm p}$}}% +\newcommand\micron{\mbox{$\mu$m}}% +\def\farcm@apj{% + \mbox{.\kern -0.7ex\raisebox{.9ex}{\scriptsize$\prime$}}% +}% +\def\farcs@apj{% + \mbox{% + \kern 0.13ex.% + \kern -0.95ex\raisebox{.9ex}{\scriptsize$\prime\prime$}% + \kern -0.1ex% + }% +}% + + +\newcommand\ion[2]{#1$\;${% +\ifx\@currsize\normalsize\small \else +\ifx\@currsize\small\footnotesize \else +\ifx\@currsize\footnotesize\scriptsize \else +\ifx\@currsize\scriptsize\tiny \else +\ifx\@currsize\large\normalsize \else +\ifx\@currsize\Large\large +\fi\fi\fi\fi\fi\fi +\rmfamily\@Roman{#2}}\relax}% + +\renewcommand\case[2]{\mbox{$\frac{#1}{#2}$}}% +\renewcommand\slantfrac{\case}% +\newcommand\onehalf{\slantfrac{1}{2}}% +\newcommand\onethird{\slantfrac{1}{3}}% +\newcommand\twothirds{\slantfrac{2}{3}}% +\newcommand\onequarter{\slantfrac{1}{4}}% +\newcommand\threequarters{\slantfrac{3}{4}}% +\newcommand\ubvr{\mbox{$U\!BV\!R$}}%% UBVR system +\newcommand\ub{\mbox{$U\!-\!B$}}% % U-B +\newcommand\bv{\mbox{$B\!-\!V$}}% % B-V +\renewcommand\vr{\mbox{$V\!-\!R$}}% % V-R +\newcommand\ur{\mbox{$U\!-\!R$}}% % U-R + +%% need this change so that it works correctly in tables: +{\catcode`\$=\active +\gdef\nodata{ ~$\cdots$~ }}% + +\newcommand\diameter{\ooalign{\hfil/\hfil\crcr\mathhexbox20D}}% +\newcommand\degr{\arcdeg}% +\newcommand\Sun{\sun}% +\newcommand\Sol{\sun}% +\newcommand\sun{\odot}% +\newcommand\Mercury{\astro{\char1}}% Mercury symbol, "1" +\newcommand\Venus{\astro{\char2}}% Venus symbol, "2" +\newcommand\Earth{\earth}% +\newcommand\Terra{\earth}% +\newcommand\earth{\oplus}% +\newcommand\Mars{\astro{\char4}}% Mars symbol, "4" +\newcommand\Jupiter{\astro{\char5}}% Jupiter symbol, "5" +\newcommand\Saturn{\astro{\char6}}% Saturn symbol, "6" +\newcommand\Uranus{\astro{\char7}}% Uranus symbol, "7" +\newcommand\Neptune{\astro{\char8}}% Neptune symbol, "8" +\newcommand\Pluto{\astro{\char9}}% Pluo symbol, "9" +\newcommand\Moon{\astro{\char10}}% Moon symbol, "M" +\newcommand\Luna{\Moon}% +\newcommand\Aries{\astro{\char11}}% +\newcommand\VEq{\Aries}% vernal equinox (Aries) +\newcommand\Taurus{\astro{\char12}}% +\newcommand\Gemini{\astro{\char13}}% +\newcommand\Cancer{\astro{\char14}}% +\newcommand\Leo{\astro{\char15}}% +\newcommand\Virgo{\astro{\char16}}% +\newcommand\Libra{\astro{\char17}}% +\newcommand\AEq{\Libra}% autumnal equinox (Libra) +\newcommand\Scorpius{\astro{\char18}}% +\newcommand\Sagittarius{\astro{\char19}}% +\newcommand\Capricornus{\astro{\char20}}% +\newcommand\Aquarius{\astro{\char21}}% +\newcommand\Pisces{\astro{\char22}}% + + +\newcommand\sbond{\chem@bnd{\@sbnd}}% +\newcommand\dbond{\chem@bnd{\@dbnd}}% +\newcommand\tbond{\chem@bnd{\@tbnd}}% +\def\chem@bnd#1{% + {% + \kern.1em\relax + \setbox\z@\hbox{M}% + \dimen@ii.8em\relax + \p@=.1em\relax + \dimen@.5\ht\z@\dimen@i-\dimen@ + \advance\dimen@1.5\p@\advance\dimen@i-1.0\p@ + #1% + \kern.1em\relax + }% + }% +\def\@sbnd{% + \advance\dimen@-1.5\p@\advance\dimen@i1.5\p@ + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + }% +\def\@dbnd{% + \advance\dimen@-0.5\p@\advance\dimen@i0.5\p@ + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + \advance\dimen@-1.5\p@\advance\dimen@i1.5\p@ + \hskip-\dimen@ii + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + }% +\def\@tbnd{% + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + \advance\dimen@-1.5\p@\advance\dimen@i1.5\p@ + \hskip-\dimen@ii + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + \advance\dimen@-1.5\p@\advance\dimen@i1.5\p@ + \hskip-\dimen@ii + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + }% + +%\newcommand\anchor[2]{#2}% +%\renewcommand\url{\@dblarg\@url}% +%\def\@url[#1]{\anchor{#1}}% + +\let\jnl@style=\rmfamily +\def\ref@jnl#1{{\jnl@style#1}}% +\newcommand\aj{\ref@jnl{AJ}}% % Astronomical Journal +\newcommand\psj{\ref@jnl{PSJ}}% % Planetary Science Journal +\newcommand\araa{\ref@jnl{ARA\&A}}% % Annual Review of Astron and Astrophys +\renewcommand\apj{\ref@jnl{ApJ}}% % Astrophysical Journal +\newcommand\apjl{\ref@jnl{ApJL}} % Astrophysical Journal, Letters +\newcommand\apjs{\ref@jnl{ApJS}}% % Astrophysical Journal, Supplement +\renewcommand\ao{\ref@jnl{ApOpt}}% % Applied Optics +\newcommand\apss{\ref@jnl{Ap\&SS}}% % Astrophysics and Space Science +\newcommand\aap{\ref@jnl{A\&A}}% % Astronomy and Astrophysics +\newcommand\aapr{\ref@jnl{A\&A~Rv}}% % Astronomy and Astrophysics Reviews +\newcommand\aaps{\ref@jnl{A\&AS}}% % Astronomy and Astrophysics, Supplement +\newcommand\azh{\ref@jnl{AZh}}% % Astronomicheskii Zhurnal +\newcommand\baas{\ref@jnl{BAAS}}% % Bulletin of the AAS +\newcommand\icarus{\ref@jnl{Icarus}}% % Icarus +\newcommand\jaavso{\ref@jnl{JAAVSO}} % The Journal of the American Association of Variable Star Observers +\newcommand\jrasc{\ref@jnl{JRASC}}% % Journal of the RAS of Canada +\newcommand\memras{\ref@jnl{MmRAS}}% % Memoirs of the RAS +\newcommand\mnras{\ref@jnl{MNRAS}}% % Monthly Notices of the RAS +\renewcommand\pra{\ref@jnl{PhRvA}}% % Physical Review A: General Physics +\renewcommand\prb{\ref@jnl{PhRvB}}% % Physical Review B: Solid State +\renewcommand\prc{\ref@jnl{PhRvC}}% % Physical Review C +\renewcommand\prd{\ref@jnl{PhRvD}}% % Physical Review D +\renewcommand\pre{\ref@jnl{PhRvE}}% % Physical Review E +\renewcommand\prl{\ref@jnl{PhRvL}}% % Physical Review Letters +\newcommand\pasp{\ref@jnl{PASP}}% % Publications of the ASP +\newcommand\pasj{\ref@jnl{PASJ}}% % Publications of the ASJ +\newcommand\qjras{\ref@jnl{QJRAS}}% % Quarterly Journal of the RAS +\newcommand\skytel{\ref@jnl{S\&T}}% % Sky and Telescope +\newcommand\solphys{\ref@jnl{SoPh}}% % Solar Physics +\newcommand\sovast{\ref@jnl{Soviet~Ast.}}% % Soviet Astronomy +\newcommand\ssr{\ref@jnl{SSRv}}% % Space Science Reviews +\newcommand\zap{\ref@jnl{ZA}}% % Zeitschrift fuer Astrophysik +\renewcommand\nat{\ref@jnl{Nature}}% % Nature +\newcommand\iaucirc{\ref@jnl{IAUC}}% % IAU Cirulars +\newcommand\aplett{\ref@jnl{Astrophys.~Lett.}}% % Astrophysics Letters +\newcommand\apspr{\ref@jnl{Astrophys.~Space~Phys.~Res.}}% % Astrophysics Space Physics Research +\newcommand\bain{\ref@jnl{BAN}}% % Bulletin Astronomical Institute of the Netherlands +\newcommand\fcp{\ref@jnl{FCPh}}% % Fundamental Cosmic Physics +\newcommand\gca{\ref@jnl{GeoCoA}}% % Geochimica Cosmochimica Acta +\newcommand\grl{\ref@jnl{Geophys.~Res.~Lett.}}% % Geophysics Research Letters +\renewcommand\jcp{\ref@jnl{JChPh}}% % Journal of Chemical Physics +\newcommand\jgr{\ref@jnl{J.~Geophys.~Res.}}% % Journal of Geophysics Research +\newcommand\jqsrt{\ref@jnl{JQSRT}}% % Journal of Quantitiative Spectroscopy and Radiative Trasfer +\newcommand\memsai{\ref@jnl{MmSAI}}% % Mem. Societa Astronomica Italiana +\newcommand\nphysa{\ref@jnl{NuPhA}}% % Nuclear Physics A +\newcommand\physrep{\ref@jnl{PhR}}% % Physics Reports +\newcommand\physscr{\ref@jnl{PhyS}}% % Physica Scripta +\newcommand\planss{\ref@jnl{Planet.~Space~Sci.}}% % Planetary Space Science +\newcommand\procspie{\ref@jnl{Proc.~SPIE}}% % Proceedings of the SPIE + +\newcommand\actaa{\ref@jnl{AcA}}% % Acta Astronomica +\newcommand\caa{\ref@jnl{ChA\&A}}% % Chinese Astronomy and Astrophysics +\newcommand\cjaa{\ref@jnl{ChJA\&A}}% % Chinese Journal of Astronomy and Astrophysics +\newcommand\jcap{\ref@jnl{JCAP}}% % Journal of Cosmology and Astroparticle Physics +\newcommand\na{\ref@jnl{NewA}}% % New Astronomy +\newcommand\nar{\ref@jnl{NewAR}}% % New Astronomy Review +\newcommand\pasa{\ref@jnl{PASA}}% % Publications of the Astron. Soc. of Australia +\newcommand\rmxaa{\ref@jnl{RMxAA}}% % Revista Mexicana de Astronomia y Astrofisica + +%% added feb 9, 2016 +\newcommand\maps{\ref@jnl{M\&PS}}% Meteoritics and Planetary Science +\newcommand\aas{\ref@jnl{AAS Meeting Abstracts}}% American Astronomical Society Meeting Abstracts +\newcommand\dps{\ref@jnl{AAS/DPS Meeting Abstracts}}% American Astronomical Society/Division for Planetary Sciences Meeting Abstracts + + + +\let\astap=\aap +\let\apjlett=\apjl +\let\apjsupp=\apjs +\let\applopt=\ao + +\newcommand\ulap[1]{\vbox\@to\z@{{\vss#1}}}% +\newcommand\dlap[1]{\vbox\@to\z@{{#1\vss}}}% + + +\newcounter{table@save} + +%% March 25, 2019 +%% Old v5.2 way, From Greg, This allows a number like 33N to be used +%% for a table, and the cross-references will work correctly +\newcommand\tablenum[1]{% + \def\thetable{#1}% + \xdef\@currentlabel{\thetable} +\global\advance\c@table-1\relax +}% + +\let\savetablenum\tablenum + +\def\tabletypesize#1{\gdef\currtabletypesize{#1} +\def\@table@type@size{#1}}% + +\tabletypesize{\small} +\let\tablefontsize=\tabletypesize % for compatibility with old documents + +\gdef\@tablecaption{} +\def\tablecaption#1{\gdef\@tablecaption{#1}} + +\def\LT@endpbox{% + \@finalstrut\@arstrutbox + \egroup + \the\LT@p@ftn + \global\LT@p@ftn{}% + \hfil} + +%% Used for longtable +\def\LT@makecaption#1#2#3{% + \LT@mcol\LT@cols c{\hbox to\z@{\hss\parbox[t]\LTcapwidth +{% +\xdef \@currentlabel{\thetable} + \sbox\@tempboxa{\small #2. +%% disable trackchanges commands here, so they aren't entered 2 times: +\let\added\relax +\let\deleted\relax +\let\replaced\relax +#3}% + \ifdim\wd\@tempboxa>\hsize + \small#2. #3% + \else + \hbox to\hsize{\hfil\box\@tempboxa\hfil}% + \fi + \endgraf\vskip\baselineskip}% + \hss}} +}%% + +\let\LT@makecaption@rtx=\LT@makecaption % to fight redefinition in Revtex-4.1 + +\def\xfigure{figure} +%% from book.cls/ used?? +\long\def\@makecaption#1#2{% + \vskip\abovecaptionskip +%% \small added to keep currtabletypesize from determining size of caption + \sbox\@tempboxa{\small +%% disable trackchanges commands here, so they aren't entered 2 times: +\let\added\relax +\let\deleted\relax +\let\replaced\relax +{\bf #1.} #2}% + \ifdim \wd\@tempboxa >\hsize +\small +{\bf #1.} #2\par + \else + \global \@minipagefalse + \hb@xt@\hsize{\hfill\box\@tempboxa\hfill}% + \fi + \vskip\belowcaptionskip +} + +\newdimen\@abovenoteskip +\newcommand\tablerefs[1]{\ifdim\@abovenoteskip=0pt\global\@abovenoteskip=10pt\fi +{\small\@tableref{\parfillskip\z@ plus1fil\relax #1\endgraf}}}% + +\def\@tableref#1{% + \par + \vspace*{3ex}% + {%\parbox{\pt@width} %%%% + {\hskip1em\rm References. --- #1}\par}% +}% + +%% march 2019, added \it to tablenotemark +\global\def\tablenotemark#1{{\normalfont\textsuperscript{\normalsize\it #1}}} +\global\def\tablenotetext#1#2{\footnotetext[#1]{\currtabletypesize\relax#2}} + +%% redefined by AH below, since it wasn't working with tabular table +\global\def\tablenotetext#1#2{\vskip-8pt\vskip1sp\flushleft{\currtabletypesize +\noindent\hskip1em $^{#1}$ #2}\vskip1sp} + +%% this version of \tablehead doesn't seem to be used, so set to \xyztablehead{} +\def\xyztablehead#1{\@table@not@headedfalse% + \kill + \caption{\\% + \@tablecaption\gdef\@currentlabel{\thetable}(0)} + \\\hline\hline% + #1\vrule height 12pt depth 10pt width 0pt\relax +\hskip\tabcolsep\\[.7ex] + \hline\\[-1.5ex] + \endfirsthead + \caption[]{--- \emph{Continued}}\\ + \hline + \hline\\[-1.7ex] + #1\hskip\tabcolsep\\[.7ex] + \hline\\[-1.5ex] + \endhead + \hline + \endfoot% +} + +\newif\if@table@not@headed + +\newlength{\table@note@skip} +\setlength{\table@note@skip}{0.5ex} +\newlength{\deluxe@table@width} +\newlength{\@d@t@a} +\newcounter{deluxe@table@num} +\newdimen\LTcapwidth + +%% \ignorespaces necessary ++== depth 6pt was depth 3pt, == added height 12pt, nov 2017 +\def\colhead#1{\multicolumn{1}{c}{\vrule depth 6pt height 12pt width +0pt\relax#1}\ignorespaces} +\def\twocolhead#1{\multicolumn{2}{c}{\hss\vrule depth 6pt height 12pt width +0pt\relax#1\hss}\ignorespaces} +\def\nocolhead#1{\multicolumn{1}{h}{}\ignorespaces} +\def\dcolhead#1{\multicolumn{1}{c}{$\vrule depth 6pt height12pt +width0pt\relax#1$}\ignorespaces} + +%\newcounter{LT@tables} +\def\tablewidth#1{% + \ifdim#1=\z@ + \else + \gdef\@d@t@@flag{1} + \if@filesw\immediate\write\@auxout{% + \gdef\expandafter\noexpand + \csname deluxe@table@width@\romannumeral\c@LT@tables\endcsname + {#1}} + \fi + \fi +} + + +\def\save@natural@width{% + \ifnum\@d@t@@flag=0 + \setlength{\@d@t@a}{0pt}% + \let\@d@t@b=\LT@entry% + \def\LT@entry##1##2{\addtolength{\@d@t@a}{##2}% + }% + \expandafter\csname LT@\romannumeral\c@deluxe@table@num\endcsname + \setlength{\@d@t@a}{-\@d@t@a} + \tablewidth{\the\@d@t@a} + \def\LT@entry{\@d@t@b} + \fi +} + +\def\lt@expand@linewidth@one{\setlength\LTleft{0pt}\setlength\LTright{0pt}} +\def\lt@expand@linewidth@two{@{\extracolsep{0pt plus 1filll}}} + +\def\find@table@width{% +%%% set table width using aux file and command \tablewidth + \setcounter{deluxe@table@num}{\c@LT@tables} + \refstepcounter{deluxe@table@num} + \expandafter\ifx\csname deluxe@table@width@\romannumeral\c@deluxe@table@num\endcsname\relax + \def\@d@t@{0.999\linewidth} + \else + \edef\@d@t@{\expandafter\csname deluxe@table@width@\romannumeral\c@deluxe@table@num\endcsname} + \fi + \ifdim\@d@t@<\z@% then natural width is used + \setlength{\deluxe@table@width}{-\@d@t@} + \setlength{\LTcapwidth}{-\@d@t@} + \def\lt@expand@linewidth{\relax} + \def\lt@expand@linewidth@{} + \else% we will enclose table in the minipage of the given width and make + % longtable to span the full minipage width + \ifdim\@d@t@>\z@\else\def\@d@t@{0.999\linewidth}\fi + \setlength{\deluxe@table@width}{\@d@t@} + \setlength{\LTcapwidth}{\@d@t@} + \def\lt@expand@linewidth{\lt@expand@linewidth@one} + \def\lt@expand@linewidth@{\lt@expand@linewidth@two} + \fi +} + +\newlength{\abovedeluxetableskip} +\newlength{\belowdeluxetableskip} +\setlength{\abovedeluxetableskip}{0pt} +\setlength{\belowdeluxetableskip}{0pt} +\setlength{\tabcolsep}{5pt} + +\setlength\doublerulesep{1.5pt} +\newdimen\lastrowheight +\def\set@last@row@height{\setlength{\lastrowheight}{\ht\strutbox}\addtolength{\lastrowheight}{\dp\strutbox}\setlength{\lastrowheight}{-\arraystretch\lastrowheight}} + +\let\tableline=\colrule % Revtex said: Command \tableline is obsolete; Use \colrule instead.. + +%% +\newtoks\DT@p@ftn +\global\def\xtablenotetext@DT#1#2{ + \edef\@tempa{\the\DT@p@ftn\noexpand\tablenotemark{#1}~} + \global\DT@p@ftn\expandafter{\@tempa{\@table@type@size#2}\par}}% + +%%% AH %%%%%%%%%%%%%%%%%%%%% +\let\savedollar$ +\catcode`\$=\active +\let$\savedollar + +%% + +\def\resetdecimals{\global\let\zdoit\relax\global\let\ddoit\relax} + +\def\tableheadfrac#1{} +\newcount\pt@column +\newcount\pt@ncol + +\newcommand\tablecolumns[1]{% + \pt@column=#1\relax + \pt@ncol=#1\relax + \global\let\pt@addcol\@empty +}% + +%% from older version, probably can delete: +\def\@tablecom#1{% + \vspace*{\table@note@skip} +\par +{\parbox{\linewidth}{\hskip1em\rmfamily {\@eapj@cap@font Note}. --- #1}\par}% +}% +\def\@tableref#1{% + \vspace*{\table@note@skip} +\par +{\parbox{\linewidth}{\hskip1em\rmfamily {\@eapj@cap@font References}. --- #1}\par}% +}% +\def\spew@tblnotes{% + \@ifx@empty\tblref@list{}{% + \@tablenotes{\tblref@list}% + \vspace*{\table@note@skip}% + \global\let\tblref@list\@empty + }% + \@ifx@empty\tblnote@list{}{% + \@tablenotes{\tblnote@list}% + \vspace*{\table@note@skip}% + \global\let\tblnote@list\@empty + } + \the\DT@p@ftn% +}% + +%% for notes on emulateapj please see http://hea-www.harvard.edu/~alexey/emulateapj +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% End of code taken from emulateapj.cls %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + + +%%% New as of august 2015: + +%% These commands requested AAS +\newcommand{\noprint}[1]{} +\newcommand{\figsetstart}{{\bf Fig. Set} } +\newcommand{\figsetend}{} +\newcommand{\figsetgrpstart}{} +\newcommand{\figsetgrpend}{} +\newcommand{\figsetnum}[1]{{\bf #1.}} +\newcommand{\figsettitle}[1]{ {\bf #1}} +\newcommand{\figsetgrpnum}[1]{\noprint{#1}} +\newcommand{\figsetgrptitle}[1]{\noprint{#1}} +\newcommand{\figsetplot}[1]{\noprint{#1}} +\newcommand{\figsetgrpnote}[1]{\noprint{#1}} + +\usepackage{url} +%% if we take away the xx before UrlBreaks we will get a url that breaks +%% at any letter or number. It might be better to break only at / however... +\expandafter\def\expandafter\xxUrlBreaks\expandafter{\UrlBreaks% save the current one + \do\a\do\b\do\c\do\d\do\e\do\f\do\g\do\h\do\i\do\j% + \do\k\do\l\do\m\do\n\do\o\do\p\do\q\do\r\do\s\do\t% + \do\u\do\v\do\w\do\x\do\y\do\z\do\A\do\B\do\C\do\D% + \do\E\do\F\do\G\do\H\do\I\do\J\do\K\do\L\do\M\do\N% + \do\O\do\P\do\Q\do\R\do\S\do\T\do\U\do\V\do\W\do\X% + \do\Y\do\Z\do\1\do\2\do\3\do\4\do\5\do\6\do\7\do\8\do\9} + + +%% for tables continuing over pages +\usepackage{longtable} + +%% for editing changes +\usepackage{xcolor} +% hyperref link defaults to "blue" (0000ff) as this matches our publisher produced pdf style +\definecolor{xlinkcolor}{cmyk}{1,1,0,0} + + +\PassOptionsToPackage{hyphens}{url} +%% In response to request from AAS + \usepackage[bookmarks=true, % show bookmarks bar?/ Changed March 22, 2019 for + % improved accessibility + pdfnewwindow=true, % links in new window + colorlinks=true, % false: boxed links; true: colored links + linkcolor=blue, % color of internal links + citecolor=blue, % color of links to bibliography +filecolor=xlinkcolor, % color of file links +urlcolor=blue, % color of external links +final=true, + ]{hyperref} + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%% Additions to AASTeX by Amy Hendrickson, TeXnology Inc, August 17, 2015 + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Table Tools, written by Amy Hendrickson +%% for American Astronomical Society +%% August 17, 2015 +%% array package is necessary: +\usepackage{array} + +%%%%%%%% +%% 1) h in table preamble will makes text in that column ignored. + +%%%%%%%% +%% 2) uppercase C L or R will make those columns in math mode. + +%%%%%%%% +%% 3) \begin{splittabular}{}...\end{splittabular} +%% `B' in the preamble will show where the table should be broken. It may +%% be used once in a preamble to break the table into two parts, or +%% two times in a preamble to break the table into three parts. + +%% The resulting table will position left half of table above right half of table. + +%% Care should be taken with \multicolumn so that it won't be broken between +%% the two parts of the table. You may need to shorten the \multicolumn argument +%% for number of columns to be appropriate to the number of columns in +%% the new split table. + +%% In this example, for instance, we start with: +%% \begin{tabular}{ccccccc} +%% \multicolumn{7}{c}{\textsc{Table 1}} +%% and change it to: +%% \begin{splittabular}{ccccBccc} +%% \multicolumn{4}{c}{\textsc{Table 1}}\\ +%% +%% If you'd like to have a table number in the second half of the table, +%% you can ask for a second multicolumn command that will position at the +%% top of the second half of the table: +%% +%% \begin{splittabular}{ccccBccc} +%% \multicolumn{4}{c}{\textsc{Table 1}}&\multicolumn{3}{c}{\textsc{Table 1, Continued}}\\ +%% +%% You can do the same for the caption, and give a Continued caption for +%% the second half of the table. Originally: +%% \multicolumn{7}{c}{\textsc{Log of \textit{HST} Observations for +%% NGC~6388}} +%% Now, changed so that we get a caption on both halves of the table: +%% \multicolumn{4}{c}{\textsc{Log of \textit{HST} Observations for +%% NGC~6388}}&\multicolumn{3}{c}{\textsc{Log of \textit{HST} Observations for +%% NGC~6388, Continued}}\\ +%% +%% Similarly, you can rearrange table notes to appear at the bottom of +%% the appropriate half of the table. For instance, starting with this, +%% which would make table notes both appear at the bottom of the top half +%% of the table: +%% \multicolumn{4}{l}{\small{$\dagger$ Average distance of data set from +%% cluster center.}}\\ +%% \multicolumn{4}{l}{$^{\rm a}$SNAP program.}\\ +%% +%% We may substitute the following: +%% \multicolumn{4}{l}{$^{\rm a}$SNAP program.}&\multicolumn{3}{l}{\small{$\dagger$ Average distance of data set from +%% cluster center.}}\\ +%% +%% Which will produce the first endnote underneath the top half of the +%% table, and the second underneath the bottom half. +%% +%% Another option would be to have both endnotes appear below the bottom +%% half of the table. Easily done: +%% &&&&\multicolumn{3}{l}{$^{\rm a}$SNAP program.}\\ +%% &&&&\multicolumn{3}{l}{\small{$\dagger$ Average distance of data set from +%% cluster center.}}\\ +%% %% %% %% %% %% %% + +%%%%%%%% +%% 4) \colnumbers will make line with column numbers automatic. It will work with splittabular +%% and splitdeluxetable as well as tabular. +%% To use: type in \colnumbers within the table whereever you'd like it to appear, typically +%% underneath the column headers, before the lines of data. + +%%%%%%%% +%% 5) Easy Decimal numbering +%% How to make decimal numbers in tables line up on the period: + +%% Use D (for decimal column) in table preamble for every decimal number. The decimal +%% numbers will use two columns, one for the left part of the decimal +%% number and one for the right part. + +%% D may be used more than once in a table preamble. + +%% If you want to type in a column header over the decimal +%% numbers, please use \multicolumn2c{} to span both columns. + +%% After the column headers, to start decimal numbering, +%% type in \decimals in the body of the table. + +%% When entering decimal numbers +%% remember to leave a space after the decimal number, before the following &. +%% For instance: &22.3 &35.96 \\ + +%% If you'd like an empty entry, please supply a period and a space: & . &. You +%% will not see the period in the resulting table. + +%% example: +% \begin{tabular}{rDD} +% \hline +% &&&\multicolumn2c{\bf More}\\ +% &\multicolumn2c{\bf Decimals}&\multicolumn2c{\bf Decimals}\\ +% \hline +% \hline +% \decimals +% one& . &34.2 \\ +% two &567.0 &21345 \\ +% three&.0 &62.5 \\ +% four&245 &5034.349923 \\ +% five&21 & \\ +% six& &21.6 +% \end{tabular} +%% +% Decimal numbering works within \begin{splittabular}...\end{splittabular} +% \begin{splitdeluxetable} and \end{splitdeluxetable} for tables broken into two +% or three parts. \colnumbers will number the columns counting both sides +% of the decimal number as one column; \tablehead{\colhead{}...} will make +% the column headers position above the two columns used for one decimal +% number as well. +% +% Decimal numbers will be in math mode so that plus and minus signs are printed +% correctly, expressions like `$\pm$ 1.2' or `\pm 1.2', will both work +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +\let\savedollar$ +\catcode`\$=\active + +\let\savetabular\tabular +\def\tabular{\catcode`\&=\active\relax\catcode`\$=\active\relax\hskip\movetableright +\savetabular} +\long\gdef\eatone{\setbox0=\hbox\bgroup\savedollar\let$\relax} +\gdef\endeatone{\savedollar\egroup\hskip-2\tabcolsep} + +%% Hide, important because it allows us to split tables horizontally +\newcolumntype{h}{>\eatone c<\endeatone} + +\newcolumntype{C}{>{\bgroup\savedollar\let$\relax}c<{\savedollar\egroup}} +\newcolumntype{L}{>{\bgroup\savedollar\let$\relax}l<{\savedollar\egroup}} +\newcolumntype{R}{>{\bgroup\savedollar\let$\relax}r<{\savedollar\egroup}} + +\newcolumntype{B}{>\eatone c<\endeatone} %% used for \splittabular to indicate break in + %% two or three parts of table + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%% Split tables into 2 or 3 parts; stack the parts +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%% Process table preamble + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Count number of columns in preamble + +\newcount\colcount +\newcount\firstcolcount +\newcount\secondcolcount +\newcount\thirdcolcount +\newcount\columncount + +%% \makeatother is necessary to keep @ from being treated as a letter +%% when counting the number of columns in table. +\makeatother +\def\xD{D} +\def\xaster{*} +\newcount\howmanyDs +\newcount\firsthowmanyDs +\newcount\secondhowmanyDs + +\newif\ifD + +\def\countcols#1{\ifcat#1c +\global\advance\colcount by 1\relax\fi +%% +\def\lookforD{#1} +\ifx\lookforD\xD +\global\advance\howmanyDs by 1 +\global\advance\colcount by1\relax +\fi +%% +\futurelet\next\lookatnext +} +\makeatletter + +\def\xeatone#1{\countcols} +\def\xrelax{\relax} + +%% second conditional deals with expressions like @{} in +%% the preamble. +\def\lookatnext{\if\next\xrelax\let\go\relax +\else +\ifx\next\bgroup\let\go\xeatone\else +\let\go\countcols\fi\fi\go} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% reset line counting at \\ + +%% arraycr redefined to match revtex4-1 +\def\new@arraycr{\relax +\global\columncount=0\relax +\global\colheadcount=0\relax +\iffalse {\fi \ifnum 0=`}\fi \@ifstar {\global \@tbpen \@M \@xarraycr} +{\global \@tbpen \intertabularlinepenalty \@xarraycr}} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Redefining & is necessary to get around \omit in \multicolumn, +%% which prevents @{} from being used to change the meaning of multicolumn. +%% Now column number and top or bottom table is used to determine whether +%% multicolumn should be turned on or off. +\let\saveampersand& + +\newif\iffirstbox +\newif\ifsecondbox +\newif\ifthirdbox + +\long\gdef\CheckNumberAndSwitch{\unskip\global\advance\columncount by 1\relax% +\saveampersand} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Parse and count preamble + +\def\catchfirstpreamble#1B#2Z{%firstpreamble +\def\leftpreamble{#1\relax} +\colcount=0 +\global\howmanyDs=0\relax +\expandafter\countcols\leftpreamble +\global\firstcolcount\the\colcount +\global\firsthowmanyDs\the\howmanyDs +\ifnum\firstcolcount>25 +\typeout{^^J +----------------------------------------------------- +^^J +Warning! +^^J^^J +Too many columns in first part of table! +^^J^^J +Maximum number of columns in each part of the table is 25. Each `D' counts as two columns. +^^J +----------------------------------------------------- +}\fi +\global\howmanyDs=0\relax +\global\colcount=0\relax +\newcolumntype{A}{#1}} + +\def\catchsecondpreamble#1B#2Z{%secondpreamble +\def\rightpreamble{#2\relax} +\colcount=0 +\expandafter\countcols\rightpreamble +\global\secondcolcount\colcount +\global\secondhowmanyDs\the\howmanyDs +\ifnum\secondcolcount>25 +\typeout{^^J----------------------------------------------------- +^^J +Warning! +^^J^^J +Too many columns in second part of table! +^^J^^J +Maximum number of columns in each part of the table is 25. Each `D' counts as two columns. +^^J +----------------------------------------------------- +}\fi +\global\totalcolumns=\firstcolcount +\global\advance\totalcolumns by \secondcolcount +\global\colcount=0\relax +\newcolumntype{Z}{#2}} + + +\def\catchsecondofthreepreamble#1B#2B#3Z{%secondpreamble +\def\rightpreamble{#2\relax} +\colcount=0 +\howmanyDs=0 +\expandafter\countcols\rightpreamble +\global\secondcolcount\colcount +\global\secondhowmanyDs\the\howmanyDs +\global\totalcolumns=\firstcolcount +\global\advance\totalcolumns by \secondcolcount +\global\colcount=0\relax +\newcolumntype{Z}{#2}} + + +\def\catchthirdpreamble#1B#2B#3Z{%firstpreamble +\def\thirdpreamble{#3} +\colcount=0 +\expandafter\countcols\thirdpreamble +\global\thirdcolcount\the\colcount +\global\advance\totalcolumns by \thirdcolcount +\global\colcount=0\relax +\newcolumntype{z}{#3}} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Define splittabular/endsplittabular + +\newcount\PartsOfTable +\newif\ifbreaktab + +\def\checkforB #1B#2B#3B{ +%% defaults, may be used in \colnumbers +\gdef\tabfullpreamble{#1#2#3\relax} +\gdef\firstpreamble{#1} +\gdef\secondpreamble{#2} +\gdef\thirdpreamble{#3} +\ifx\thirdpreamble\empty +\global\PartsOfTable=2 +\else +\global\PartsOfTable=3 +\fi +} + +\def\lookforD#1{\def\zone{#1}\ifx\zone\xD +\global\Dtrue\else\Dfalse\fi} + +\newcount\columnoneandtwo +\newif\ifdonullmulticol + +\newcount\colnumsused +\newcount\loopnum + +\catcode`\&=\active +\let&\CheckNumberAndSwitch +\let$\savedollar + +%sss +\def\splittabular{\catcode`\&=\active +\catcode`\$=\active +\global\colnumbersonfalse +\let\colnumbers\savesplitplaincolnumbers +\let\splitdecimalcolnumbers\savesplitdecimalcolnumbers +\def\decimalcolnumbers{\splitdecimalcolnumbers} +\xsplittabular} + +\def\xsplittabular#1#2\end{{ +\global\firsttimetrue +\let&\CheckNumberAndSwitch +\let$\savedollar +%%% +\def\endtabular{\endarray +\global\let\zdoit\relax +\global\let\ddoit\relax +\global\Dfalse} +\setbox0=\hbox{\def\firstarg{#1}\expandafter\lookforD\firstarg} +\PartsOfTable=0 +\def\tempfullpreamble{#1BB} +\setbox0=\hbox{\expandafter\checkforB\tempfullpreamble} +%% Now PartsOfTable is either =2 or 3 +%% +\global\colnumsused=0 +\global\breaktabtrue +\global\colcount=0 +%% +\ifnum\PartsOfTable=3 +\let\multicolumn\threebreakmulticolumn +\else +\let\multicolumn\breakmulticolumn +\fi +%% +\def\one{#1Z}%% full preamble +\ifnum\PartsOfTable=3 +\expandafter\catchfirstpreamble\one +\expandafter\catchsecondofthreepreamble\one +\expandafter\catchthirdpreamble\one +\makefirstdummycolumns %f +\makeseconddummycolumns %F +\makethirddummycolumns %E +\else %% PartsOfTable=2 +\expandafter\catchfirstpreamble\one +\expandafter\catchsecondpreamble\one +\makefirstdummycolumns %f +\makeseconddummycolumns %F +\fi +%%% +\global\columncount=0 +\ifnum\PartsOfTable=3 +%% For table divided into three parts !! +\firstboxtrue\secondboxfalse\thirdboxfalse +% +\setbox\firsttablebox=\hbox{% +\begin{tabular}{AFE}% +#2\crcr +\end{tabular}} +% +\hbox to \hsize{\hss\unhbox\firsttablebox\hss} +\vskip6pt +\hrule +\vskip6pt +\global\columncount=0 +\firstboxfalse\secondboxtrue\thirdboxfalse +\ifcolnumberson +\let\colnumbers\xplain +\setbox\secondtablebox=\hbox{% +\begin{tabular}{fZE}% fZE +#2\crcr\end{tabular}} +\else +\setbox\secondtablebox=\hbox{ +\begin{tabular}{fZE}% fZE +#2 +\end{tabular}} +\fi +\hbox to \hsize{\hss\unhbox\secondtablebox\hss} +%% +\vskip6pt +\hrule +\vskip6pt +\firstboxfalse\secondboxfalse\thirdboxtrue +\global\columncount=0 +\ifcolnumberson +\let\colnumbers\xplain +\setbox\thirdtablebox=\hbox{% +\begin{tabular}{fFz}% fFz +#2\crcr\end{tabular}} +\else +\setbox\thirdtablebox=\hbox{ +\begin{tabular}{fFz}% fFz +#2 +\end{tabular}} +\fi +\hbox to \hsize{\hss\unhbox\thirdtablebox\hss} +\else +%% +%% For table divided into two parts: +%% +\global\columncount=0 +\secondboxfalse + \setbox\firsttablebox=\hbox{% +\begin{tabular}{AF}% should be AF +#2 +\end{tabular} +} + \hbox to \hsize{\hss\unhbox\firsttablebox\hss} +\vskip6pt +\hrule +\vskip6pt +\global\columncount=0 +\secondboxtrue +\ifcolnumberson +\setbox\secondtablebox=\hbox{\let\colnumbers\xplain +\begin{tabular}{fZ}% should be fZ +#2 +\end{tabular} +} +\else +\setbox\secondtablebox=\hbox{ +\begin{tabular}{fZ}% should be fZ +#2 +\end{tabular} +} +\fi +\hbox to \hsize{\hss\unhbox\secondtablebox\hss} +%% +%% end of conditional testing for 2 or 3 part table: +\fi +%\global\breaktabfalse +} +\firsthowmanyDs=0 +\secondhowmanyDs=0 +\resetdecimals +\end +} + +%yyy +\def\endsplittabular{\global\firsttimefalse\global\colnumbersonfalse +\global\let\splitplaincolnumbers\savesplitplaincolnumbers +\global\breaktabfalse} + +\long\gdef\breakmulticolumn#1#2#3{% +\multispan{#1}% +\let&\CheckNumberAndSwitch +\ifsecondbox% +\ifnum\columncount<\firstcolcount% +\global\donullmulticoltrue% +\else% +\global\donullmulticolfalse% +\fi% +%%% + \else% first box +\ifnum\columncount<\firstcolcount% +\global\donullmulticolfalse% +\else% +\global\donullmulticoltrue% +\fi% +\fi% +\ifdonullmulticol% +\global\advance\colheadcount by 1\relax +\begingroup + \def\@addamp{\if@firstamp \@firstampfalse \else + \@preamerr 5\fi}% + \@mkpream{h}\@addtopreamble\@empty + \endgroup + \def\@sharp{}% +%% comment out \@arstrut to prevent blank line where multicolumn was found +%% on other parts of the table, but not on the current part. + \@arstrut +\@preamble + \null\ignorespaces +\else% +\begingroup + \def\@addamp{\if@firstamp \@firstampfalse \else + \@preamerr 5\fi}% + \@mkpream{#2}\@addtopreamble\@empty + \endgroup + \def\@sharp{#3}% + \@arstrut \@preamble + \null\ignorespaces +\fi% +\global\donullmulticolfalse% +\global\advance\columncount by #1\relax% +\global\advance\columncount-1\relax% +} + + +\long\gdef\threebreakmulticolumn#1#2#3{% +\multispan{#1}% +\columnoneandtwo=\firstcolcount\relax% +\advance\columnoneandtwo by \secondcolcount\relax% +%% +\global\donullmulticoltrue\relax% +\iffirstbox\relax% +\ifnum\columncount<\firstcolcount% +\global\donullmulticolfalse% +\fi\relax% +\ifnum\columncount=\firstcolcount\relax% +\donullmulticoltrue\fi\relax% +\else\relax% +%% +\ifsecondbox% +\ifnum\columncount=\firstcolcount\relax% +\global\donullmulticolfalse\fi\relax% +\ifnum\columncount>\firstcolcount% +\ifnum\columncount<\columnoneandtwo\relax% +\global\donullmulticolfalse\relax% +\fi\fi\relax% +\else\relax% +%%% +\ifthirdbox% +\ifnum\columncount<\columnoneandtwo% +\global\donullmulticoltrue% +\else\relax% +\global\donullmulticolfalse% +\fi\relax% +\fi%% end if third box +\fi%% end if second box +\fi%% end if first box +%% +\ifdonullmulticol% +\begingroup\relax% +\global\advance\colheadcount by 1\relax% + \def\@addamp{\if@firstamp \@firstampfalse \else% + \@preamerr 5\fi}% + \@mkpream{h}\@addtopreamble\@empty% + \endgroup% + \def\@sharp{}% +%% comment out \@arstrut to prevent blank line where multicolumn was found +%% on other parts of the table, but not on the current part. + \@arstrut \@preamble% + \null\ignorespaces +\else% +\begingroup% + \def\@addamp{\if@firstamp \@firstampfalse \else% + \@preamerr 5\fi}% + \@mkpream{#2}\@addtopreamble\@empty% + \endgroup% + \def\@sharp{#3}% + \@arstrut \@preamble% + \null\ignorespaces +\fi% +\global\donullmulticolfalse% +\global\advance\columncount by #1\relax% +\global\advance\columncount-1\relax% +} + +%% First dummy columns is the part of the table that will not print, +%% in this case the first part to the left. +%%\makefirstdummycolumns +%% +%% and second dummy columns +%% \makeseconddummycolumns. +\gdef\makefirstdummycolumns{ +\ifcase\firstcolcount +\or% 1 +\newcolumntype{f}{h} % no D possible +%%%%%%%%%%%%%%%%%% +\or% 2 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hh}%% 0 + \or + \newcolumntype{f}{d} %% 1 + \fi +%%%%%%%%%%%%%%%%%% +\or% 3 + \ifcase\firsthowmanyDs% + \newcolumntype{f}{hhh}% 0 + \or% + \newcolumntype{f}{dh}% 1 + \fi% +%%%%%%%%%%%%%%%%%% +\or% 4 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhh} % 0 + \or + \newcolumntype{f}{dhh} % 1 + \or + \newcolumntype{f}{dd} % 2 + \fi +%%%%%%%%%%%%%%%%%% +\or% 5 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhh} % 0 + \or + \newcolumntype{f}{dhhh} % 1 + \or + \newcolumntype{f}{ddh} % 2 + \fi +%%%%%%%%%%%%%%%%%% +\or% 6 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhh} % 0 + \or + \newcolumntype{f}{dhhhh} % 1 + \or + \newcolumntype{f}{ddhh} % 2 + \or + \newcolumntype{f}{ddd} % 3 + \fi +%%%%%%%%%%%%%%% +\or % 7 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhh} % 1 + \or + \newcolumntype{f}{ddhhh} % 2 + \or + \newcolumntype{f}{dddh} % 3 + \fi +%%%%%%%%%%%%%%%%%% +\or % 8 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhh} % 2 + \or + \newcolumntype{f}{dddhh} % 3 + \or + \newcolumntype{f}{dddd} % 4 + \fi +%%%%%%%%%%%%%%%%%% +\or % 9 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhh} % 2 + \or + \newcolumntype{f}{dddhhh} % 3 + \or + \newcolumntype{f}{ddddh} % 4 + \fi +%%%%%%%%%%%%%%%%%% +\or %10 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhh} % 3 + \or + \newcolumntype{f}{ddddhh} % 4 + \or + \newcolumntype{f}{ddddd} % 5 + \fi +%%%%%%%%%%%%%%%%%% +\or % 11 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhh} % 4 + \or + \newcolumntype{f}{dddddh} % 5 + \fi +%%%%%%%%%%%%%%%%%% +\or % 12 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhh} % 4 + \or + \newcolumntype{f}{dddddhh} % 5 + \or + \newcolumntype{f}{dddddd} % 6 + \fi +%%%%%%%%%%%%%%%%%% +\or %13 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhh} % 5 + \or + \newcolumntype{f}{ddddddh} % 6 + \fi +%%%%%%%%%%%%%%%%%% +\or %14 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhh} % 5 + \or + \newcolumntype{f}{ddddddhh} % 6 + \or + \newcolumntype{f}{ddddddd} % 7 + \fi +%%%%%%%%%%%%%%%%%% +\or %15 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhh} % 6 + \or + \newcolumntype{f}{dddddddh} % 7 + \fi +%%%%%%%%%%%%%%%%%% +\or %16 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhh} % 6 + \or + \newcolumntype{f}{dddddddhh} % 7 + \or + \newcolumntype{f}{dddddddd} % 8 +\fi +%%%%%%%%%%%%%%%%%% +\or %17 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhh} % 6 + \or + \newcolumntype{f}{dddddddhhh} % 7 + \or + \newcolumntype{f}{ddddddddh} % 8 +\fi +%%%%%%%%%%%%%%%%%% +\or %18 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhhh} % 6 + \or + \newcolumntype{f}{ddddddhhhh} % 7 + \or + \newcolumntype{f}{ddddddddhh} % 8 + \or + \newcolumntype{f}{ddddddddd} % 9 +\fi +%%%%%%%%%%%%%%%%%% +\or %19 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhhhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhhhh} % 6 + \or + \newcolumntype{f}{dddddddhhhhh} % 7 + \or + \newcolumntype{f}{ddddddddhhh} % 8 + \or + \newcolumntype{f}{ddddddddddh} % 9 +\fi +%%%%%%%%%%%%%%%%%% +\or %20 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhh hhhhh hhhhh hhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhhhhh} % 6 + \or + \newcolumntype{f}{dddddddhhhhhh} % 7 + \or + \newcolumntype{f}{ddddddddhhhh} % 8 + \or + \newcolumntype{f}{dddddddddhh} % 9 + \or + \newcolumntype{f}{dddddddddd} % 10 + \fi +%%%%%%%%%%%%%%%%%% +\or %21 + \ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhh hhhhh hhhhh hhhhh h} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhhhhhh} % 6 + \or + \newcolumntype{f}{dddddddhhhhhhh} % 7 + \or + \newcolumntype{f}{ddddddddhhhhh} % 8 + \or + \newcolumntype{f}{ddd ddd ddd hhh} % 9 + \or + \newcolumntype{f}{ddd ddd ddd d h} % 10 + \fi +%%%%%%%%%%%%%%%%%% +\or %22 +\ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhh hhhhh hhhhh hhhhh hh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhhhhhhh} % 6 + \or + \newcolumntype{f}{dddddddhhhhhhhh} % 7 + \or + \newcolumntype{f}{ddddddddhhhhhh} % 8 + \or + \newcolumntype{f}{ddd ddd ddd hhhh} % 9 + \or + \newcolumntype{f}{ddd ddd ddd dhh} % 10 + \or + \newcolumntype{f}{ddddddddddd} % 11 + \fi +%%%%%%%%%%%%%%%%%% +\or %23 +\ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhh hhhhh hhhhh hhhhh hhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhhhhhhhh} % 6 + \or + \newcolumntype{f}{dddddddhhhhhhhhh} % 7 + \or + \newcolumntype{f}{ddddddddhhhhhhh} % 8 + \or + \newcolumntype{f}{ddd ddd ddd hhhhh} % 9 + \or + \newcolumntype{f}{ddddddddddhhh} % 10 + \or + \newcolumntype{f}{ddddd ddddd dh} % 11 + \fi +%%%%%%%%%%%%%%%%%% +\or %24 +\ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhh hhhhh hhhhh hhhhh hhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhhhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhhhhhhhhh} % 6 + \or + \newcolumntype{f}{dddddddhhhhhhhhhh} % 7 + \or + \newcolumntype{f}{ddddddddhhhhhhhh} % 8 + \or + \newcolumntype{f}{ddd ddd ddd hhhhhh} % 9 + \or + \newcolumntype{f}{ddddddddddhhhh} % 10 + \or + \newcolumntype{f}{ddddd ddddd dhh} % 11 + \or + \newcolumntype{f}{ddddd ddddd dd} % 12 + \fi +%%%%%%%%%%%%%%%%%% +\or %25 +\ifcase\firsthowmanyDs + \newcolumntype{f}{hhhhh hhhhh hhhhh hhhhh hhhhh} % 0 + \or + \newcolumntype{f}{dhhhhhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{f}{ddhhhhhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{f}{dddhhhhhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{f}{ddddhhhhhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{f}{dddddhhhhhhhhhhhhhhh} % 5 + \or + \newcolumntype{f}{ddddddhhhhhhhhhhhhh} % 6 + \or + \newcolumntype{f}{dddddddhhhhhhhhhhh} % 7 + \or + \newcolumntype{f}{ddddddddhhhhhhhhh} % 8 + \or + \newcolumntype{f}{ddd ddd ddd hhhhhhh} % 9 + \or + \newcolumntype{f}{ddddddddddhhhhh} % 10 + \or + \newcolumntype{f}{dddddddddddhhh} % 11 + \or + \newcolumntype{f}{ddddddddddddh} % 12 + \fi +%%%%%%%%%%%%%%%%%% +\else +\typeout{^^J----------------------------------------------------- ^^J +Warning!^^J^^J +Too many Columns using in Splittabular. +^^J +25 column maximum in +each part of the table.^^J Each`T' counts as two columns. +^^J-----------------------------------------------------^^J} +\fi +} + + +%% Second dummy columns is the part of the table that will not print, +%% in this case the part to the right. +%%\makeseconddummycolumns + +\gdef\makeseconddummycolumns{% +\ifcase\secondcolcount +%0 +\or +%1 +\newcolumntype{F}{h} % no D possible +%%%%%%%%%%%%%%%%%% +\or +%2 + \ifcase\secondhowmanyDs + \newcolumntype{F}{hh}%% 0 + \or + \newcolumntype{F}{d} %% 1 + \fi +%%%%%%%%%%%%%%%%%% +\or +%3 + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhh} % 0 + \or + \newcolumntype{F}{dh} % 1 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhh} % 0 + \or + \newcolumntype{F}{dhh} % 1 + \or + \newcolumntype{F}{dd} % 2 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhh} % 0 + \or + \newcolumntype{F}{dhhh} % 1 + \or + \newcolumntype{F}{ddh} % 2 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhh} % 0 + \or + \newcolumntype{F}{dhhhh} % 1 + \or + \newcolumntype{F}{ddhh} % 2 + \or + \newcolumntype{F}{ddd} % 3 + \fi +%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhh} % 1 + \or + \newcolumntype{F}{ddhhh} % 2 + \or + \newcolumntype{F}{dddh} % 3 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhh} % 2 + \or + \newcolumntype{F}{dddhh} % 3 + \or + \newcolumntype{F}{dddd} % 4 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhh} % 2 + \or + \newcolumntype{F}{dddhhh} % 3 + \or + \newcolumntype{F}{ddddh} % 4 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhh} % 3 + \or + \newcolumntype{F}{ddddhh} % 4 + \or + \newcolumntype{F}{ddddd} % 5 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhh} % 4 + \or + \newcolumntype{F}{dddddh} % 5 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhh} % 4 + \or + \newcolumntype{F}{dddddhh} % 5 + \or + \newcolumntype{F}{dddddd} % 6 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhh} % 5 + \or + \newcolumntype{F}{ddddddh} % 6 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhh} % 5 + \or + \newcolumntype{F}{ddddddhh} % 6 + \or + \newcolumntype{F}{ddddddd} % 7 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhh} % 6 + \or + \newcolumntype{F}{dddddddh} % 7 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhh} % 6 + \or + \newcolumntype{F}{dddddddhh} % 7 + \or + \newcolumntype{F}{dddddddd} % 8 +\fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhh} % 7 + \or + \newcolumntype{F}{ddddddddh} % 8 +\fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhhh} % 7 + \or + \newcolumntype{F}{ddddddddhh} % 8 + \or + \newcolumntype{F}{ddddddddd} % 9 +\fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhhhhhhhhhhhhhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhhhh} % 7 + \or + \newcolumntype{F}{ddddddddhhh} % 8 + \or + \newcolumntype{F}{dddddddddh} % 9 +\fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhh hhhhh hhhhh hhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhhhhh} % 7 + \or + \newcolumntype{F}{ddddddddhhhh} % 8 + \or + \newcolumntype{F}{dddddddddhh} % 9 + \or + \newcolumntype{F}{dddddddddd} % 10 + \fi +%%%%%%%%%%%%%%%%%% +\or + \ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhh hhhhh hhhhh hhhhh h} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhhhhhh} % 7 + \or + \newcolumntype{F}{ddddddddhhhhh} % 8 + \or + \newcolumntype{F}{ddd ddd ddd hhh} % 9 + \or + \newcolumntype{F}{ddd ddd ddd d h} % 10 + \fi +%%%%%%%%%%%%%%%%%% +\or +\ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhh hhhhh hhhhh hhhhh hh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhhhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhhhhhhh} % 7 + \or + \newcolumntype{F}{ddddddddhhhhhh} % 8 + \or + \newcolumntype{F}{ddd ddd ddd hhhh} % 9 + \or + \newcolumntype{F}{ddddddddddhh} % 10 + \or + \newcolumntype{F}{ddddddddddd} % 11 + \fi +%%%%%%%%%%%%%%%%%% +\or +\ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhh hhhhh hhhhh hhhhh hhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhhhhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhhhhhhhh} % 7 + \or + \newcolumntype{F}{ddddddddhhhhhhh} % 8 + \or + \newcolumntype{F}{ddd ddd ddd hhhhh} % 9 + \or + \newcolumntype{F}{ddddddddddhhh} % 10 + \or + \newcolumntype{F}{ddddd ddddd dh} % 11 + \fi +%%%%%%%%%%%%%%%%%% +\or +\ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhh hhhhh hhhhh hhhhh hhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhhhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhhhhhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhhhhhhhhh} % 7 + \or + \newcolumntype{F}{ddddddddhhhhhhhh} % 8 + \or + \newcolumntype{F}{ddd ddd ddd hhhhhh} % 9 + \or + \newcolumntype{F}{ddddddddddhhhh} % 10 + \or + \newcolumntype{F}{ddddd ddddd dhh} % 11 + \or + \newcolumntype{F}{ddddd ddddd dd} % 12 + \fi +%%%%%%%%%%%%%%%%%% +\or +\ifcase\secondhowmanyDs + \newcolumntype{F}{hhhhh hhhhh hhhhh hhhhh hhhhh} % 0 + \or + \newcolumntype{F}{dhhhhhhhhhhhhhhhhhhhhhhh} % 1 + \or + \newcolumntype{F}{ddhhhhhhhhhhhhhhhhhhhhh} % 2 + \or + \newcolumntype{F}{dddhhhhhhhhhhhhhhhhhhh} % 3 + \or + \newcolumntype{F}{ddddhhhhhhhhhhhhhhhhh} % 4 + \or + \newcolumntype{F}{dddddhhhhhhhhhhhhhhh} % 5 + \or + \newcolumntype{F}{ddddddhhhhhhhhhhhhh} % 6 + \or + \newcolumntype{F}{dddddddhhhhhhhhhhh} % 7 + \or + \newcolumntype{F}{ddddddddhhhhhhhhh} % 8 + \or + \newcolumntype{F}{ddd ddd ddd hhhhhhh} % 9 + \or + \newcolumntype{F}{ddddddddddhhhhh} % 10 + \or + \newcolumntype{F}{ddddd ddddd dhhh} % 11 + \or + \newcolumntype{F}{ddddd ddddd ddh} % 12 + \fi +%%%%%%%%%%%%%%%%%% +\else +\typeout{^^J----------------------------------------------------- ^^J +Warning!^^J^^J +Too many Columns using in Splittabular. +^^J +25 column maximum in +each part of the table.^^J Each`D' counts as two columns. +^^J-----------------------------------------------------^^J} +\fi +} + +%% we don't have to worry about D's in this section, fortunately. +\gdef\makethirddummycolumns{ +\ifcase\thirdcolcount +\or\newcolumntype{E}{h} +\or\newcolumntype{E}{hh} +\or\newcolumntype{E}{hhh} +\or\newcolumntype{E}{hhhh} +\or\newcolumntype{E}{hhhhh} +\or\newcolumntype{E}{hhhhhh} +\or\newcolumntype{E}{hhhhhhh} +\or\newcolumntype{E}{hhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhhhhhhhhh} +\or\newcolumntype{E}{hhhhhhhhhhhhhhhhhhhhhhhhh} %% up to 25 columns +\else \typeout{^^J-----------------------------------------------------^^J +Warning! +^^J^^J Too many Columns in Splittabular. +^^J +25 column maximum in +each part of the table.^^J +Each `D' counts as two columns. +^^J-----------------------------------------------------^^J}\fi +} + +%%%%%%%%%%%%%%%%% +%% Colnums + +%% defaults + +\gdef\settabnumdefaults{% +\loopnum=0\relax\loop% +\ifnum\loopnum<31\relax% +\expandafter\gdef\csname tab\the\loopnum\endcsname{% +\multicolumn1{c}{\global\advance\colnumsused by 1\relax% +(\the\colnumsused)}}% +\global\advance\loopnum by1\repeat} + +%%%%%%%%%%%%%%%%%%%%%%%%% +%% this version of countcols is for \colnumbers +\newcount\totalcolumncount +\def\xH{h} + +\makeatother +\def\tabcountcols#1{\ifcat#1c +\global\advance\colcount by 1\relax\fi% +%% +\def\lookforD{#1}% +\ifx\lookforD\xD% +\expandafter\gdef\csname tab\the\colcount\endcsname{% +\multicolumn2{c}{\global\advance\colnumsused by 1\relax% +(\the\colnumsused)}}% +\fi% +\ifx\lookforD\xH% +\expandafter\gdef\csname tab\the\colcount\endcsname{% +\multicolumn1{h}{}}% +\fi% +%% +\futurelet\next\tablookatnext} + +\def\tabxeatone#1{\tabcountcols} + +%% second conditional deals with expressions like @{} in +%% the preamble. +\def\tablookatnext{\if\next\xrelax\let\xgo\relax\else% +\ifx\next\bgroup\let\xgo\tabxeatone\else\let\xgo\tabcountcols\fi\fi\xgo} +\makeatletter +%%%%%%%%%%%%%%% + +\newcount\totalcolumns +\newbox\firsttablebox +\newbox\secondtablebox +\newbox\thirdtablebox +\newif\ifdbreaktab + +%% A loop would be more elegant, of course, but using & in a loop +%% within a table column produces errors. +%% was\tabnumberline, now \colnumbers + +%% Is this test necessary? +%\newif\ifcolumnums + +\newif\ifcolnumberson +\def\deluxecolnumbers{\global\colnumbersontrue} + +\def\colnumbers{\omit\\\omit\xcolnumbers} +\def\xcolnumbers{\global\let\colnumbers\xcolnumbers% +\global\colnumbersontrue\let&\CheckNumberAndSwitch% +\global\colcount=0\relax% +\global\totalcolumncount=0\relax% +%% above here +\settabnumdefaults% +%% Now, change the columns that have `D' to be \multicolumn2c, by redefining +%% the \csname tab\endcsname +%% +\expandafter\tabcountcols\tabfullpreamble% +\global\totalcolumncount=\the\colcount\relax% +\global\colcount=0\relax% +\ifbreaktab\else\ifdbreaktab\else\global\colnumsused=0\relax\fi\fi% +%% +% +\ifdeluxe\ifbreaktab\\\else\\[-6pt]\fi%\hline% not above +\else% +\\[-14pt]\fi% +\ifcase\totalcolumncount% +\or% +\csname tab1\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&%% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname% +\or +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname% +\or%22 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname% +\or% 24 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname% +\or% 25 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname% +\or% 27 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname% +\or% 28 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname% +\or% 29 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname&% +\csname tab29\endcsname% +\or% 30 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname&% +\csname tab29\endcsname&\csname tab30\endcsname% +\else% +\typeout{^^J^^J +Sorry, more than 30 columns cannot be numbered with^^J +\string\colnumbers. Please number the columns manually.^^J +Thank you!^^J}\fi% +%\ifbreaktab +\\\hline% below, hline is wanted +%\else +\noalign{\vskip-8pt} +%\vrule height 28pt width0pt %the \vrule is in the line below colnumbers; + % it causes all the vrules on that line to grow to 28pt. + % The -14pt will cause the lower line to overlap the upper line. + % Complication, needed to add this vrule to Z and z in order to + % have it also work for split tabular. +%\fi +} + + + +\let\savecolnumbers\colnumbers + +\gdef\plaincolnumbers{% +\omit\\\omit% +\global\colnumbersontrue\let&\CheckNumberAndSwitch% +\global\colcount=0\relax% +\global\totalcolumncount=0\relax% +%% above here +\settabnumdefaults% +%% Now, change the columns that have `D' to be \multicolumn2c, by redefining +%% the \csname tab\endcsname +%% +\expandafter\tabcountcols\tabfullpreamble% +\global\totalcolumncount=\the\colcount\relax% +\global\colcount=0\relax% +\ifbreaktab\else\ifdbreaktab\else\global\colnumsused=0\relax\fi\fi% +%% +\\\ifcase\totalcolumncount% +\or% +\csname tab1\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&%% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname% +\or +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname% +\or%22 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname% +\or% 24 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname% +\or% 25 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname% +\or% 27 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname% +\or% 28 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname% +\or% 29 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname&% +\csname tab29\endcsname% +\or% 30 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname&% +\csname tab29\endcsname&\csname tab30\endcsname% +\else% +\typeout{^^J^^J +Sorry, more than 30 columns cannot be numbered with^^J +\string\colnumbers. Please number the columns manually.^^J +Thank you!^^J}\fi% +\\\hline% below, hline is wanted +\\\noalign{\vskip-30pt }%%%%% +%\vrule height 28pt width0pt %the \vrule is in the line below colnumbers; + % it causes all the vrules on that line to grow to 28pt. + % The -14pt will cause the lower line to overlap the upper line. + % Complication, needed to add this vrule to Z and z in order to + % have it also work for split tabular. +} + +\let\saveplaincolnumbers\plaincolnumbers + + +\def\splitplaincolnumbers{% +\omit\\\omit% +\xplain} + +\let\savesplitplaincolnumbers\splitplaincolnumbers + +\newif\iffirsttime +\firsttimetrue +\gdef\xplain{% +\global\let\plaincolnumbers\xplain% +\global\colnumbersontrue\let&\CheckNumberAndSwitch% +\global\colcount=0\relax% +\global\totalcolumncount=0\relax% +%% above here +\settabnumdefaults% +%% Now, change the columns that have `D' to be \multicolumn2c, by redefining +%% the \csname tab\endcsname +%% +\expandafter\tabcountcols\tabfullpreamble% +\global\totalcolumncount=\the\colcount\relax% +\global\colcount=0\relax% +\ifbreaktab\else\ifdbreaktab\else\global\colnumsused=0\relax\fi\fi% +%% +\iffirsttime +\\%\hline% above not wanted +\else +\\[-12pt]%\hline% above not wanted +\fi +\ifcase\totalcolumncount% +\or% +\csname tab1\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&%% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname% +\or +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname% +\or%22 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname% +\or% 24 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname% +\or% 25 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname% +\or% +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname% +\or% 27 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname% +\or% 28 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname% +\or% 29 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname&% +\csname tab29\endcsname% +\or% 30 +\csname tab1\endcsname&\csname tab2\endcsname&% +\csname tab3\endcsname&\csname tab4\endcsname&% +\csname tab5\endcsname&\csname tab6\endcsname&% +\csname tab7\endcsname&\csname tab8\endcsname&% +\csname tab9\endcsname&\csname tab10\endcsname&% +\csname tab11\endcsname&\csname tab12\endcsname&% +\csname tab13\endcsname&\csname tab14\endcsname&% +\csname tab15\endcsname&\csname tab16\endcsname&% +\csname tab17\endcsname&\csname tab18\endcsname&% +\csname tab19\endcsname&\csname tab20\endcsname&% +\csname tab21\endcsname&\csname tab22\endcsname&% +\csname tab23\endcsname&\csname tab24\endcsname&% +\csname tab25\endcsname&\csname tab26\endcsname&% +\csname tab27\endcsname&\csname tab28\endcsname&% +\csname tab29\endcsname&\csname tab30\endcsname% +\else% +\typeout{^^J^^J +Sorry, more than 30 columns cannot be numbered with^^J +\string\colnumbers. Please number the columns manually.^^J +Thank you!^^J}\fi% +\\\hline% below, hline is wanted +\iffirsttime +\\\noalign{\vskip-30pt}%% +%\noalign{\vskip-8pt} +\vrule height 28pt width0pt %the \vrule is in the line below colnumbers; + % it causes all the vrules on that line to grow to 28pt. + % The -14pt will cause the lower line to overlap the upper line. + % Complication, needed to add this vrule to Z and z in order to + % have it also work for split tabular. +\fi\global\firsttimefalse +} + +\def\decimalcolnumbers{\crcr\saveplaincolnumbers\\% +\noalign{\global\savetabskip\tabskip +\tabskip=0pt +\global\let\extracolsep\relax +\global\let\ddoit\saveddoit +\global\let\zdoit\savezdoit +\vskip-32pt +}{\vrule height28pt depth0pt width0pt}\relax} + +\def\splitdecimalcolnumbers{\\[-15pt]% +\savesplitplaincolnumbers +\global\colnumbersonfalse +\\\noalign{\vskip-32pt %!!! +\global\savetabskip\tabskip +\tabskip=0pt +\global\let\extracolsep\relax +\global\let\ddoit\saveddoit +\global\let\zdoit\savezdoit +}\vrule height 28pt width0pt %!!! +\global\let\splitdecimalcolnumbers\secondsplitdecimalcolnumbers} + +\def\secondsplitdecimalcolnumbers{\omit\\ +\plaincolnumbers +\global\colnumbersonfalse +\\\noalign{\vskip-26pt %!!! was -28pt +\global\savetabskip\tabskip +\tabskip=0pt +\global\let\extracolsep\relax +\global\let\ddoit\saveddoit +\global\let\zdoit\savezdoit +}\\\relax} + +\let\savesplitdecimalcolnumbers\splitdecimalcolnumbers + +%%AAA +\newif\ifdeluxestar +\expandafter\def\csname +deluxetable*\endcsname{\deluxestartrue\bgroup\floattrue +\hsize=\textwidth +\deluxetable} + +\expandafter\def\csname enddeluxetable*\endcsname{\enddeluxetable +\egroup +\null% added june 2020 +\global\colnumbersonfalse +\global\deluxedecimalsfalse +\global\deluxestarfalse +} + +\def\deluxedecimalcolnumbers{\deluxedecimalstrue\colnumbersontrue} +\def\deluxetablecaption#1{\gdef\@tablecaption{#1}} + +\newif\ifstartlongtable +\def\startlongtable{\vskip1sp\global\startlongtabletrue} + +\newif\iffloat +\def\floattable{\global\deluxestartrue\global\floattrue} + +%% for equivalent but in \begin...\end form. +\def\floatrotatetable{\global\deluxestartrue\global\floattrue} +\let\endfloatrotatetable\relax + +\def\deluxetable{\global\deluxetrue +\catcode`\&=\active +\catcode`\$=\active +%% Mar 30, 2019, to make label outside of \caption work correctly +{\advance\c@table by 1 +\xdef\@currentlabel{\thetable}} +\let\tablecaption\deluxetablecaption +\deluxetablecaption{} +%% july 2016 +% \iffloat +% \let\go\ydeluxetable +% \else\let\go\longdeluxetable\fi\go%} +%% aug 2016 +\ifstartlongtable +%% this works for both deluxetable and deluxetable*: +%% nov 2017: +\def\arraystretch{1.1} +%% March 2019 +\if@two@col\global\returntotwocoltrue\vskip1pt +\ifdeluxestar\onecolumngrid\fi\fi +%% +\ifdeluxestar +\vskip12pt +\fi +\let\go\longdeluxetable +\else +\let\go\ydeluxetable +\fi\go +} + +\def\ydeluxetable#1{% +\@ifnextchar[{\xdeluxetable{#1}}{\zdeluxetable{#1}}} + +%% +% x and z are the same, except that xdeluxetable allows optional square bracket arg, like [h]. +\def\xdeluxetable#1[#2]{\global\breaktabtrue +%% not here +\let\colnumbers\deluxecolnumbers +\global\deluxedecimalsfalse +\let\decimals\deluxedecimals +\let\decimalcolnumbers\deluxedecimalcolnumbers +\let\tablehead\ztablehead +\gdef\tabfullpreamble{#1}%<<== needed +\def\endtabular{\endarray +\global\let\zdoit\relax +\global\let\tdoit\relax +\global\Dfalse} +\global\colnumsused=0 +\global\breaktabtrue +\global\colcount=0 +%% +%%%%%%%%%%%% + \lineskiplimit=\z@ % restore default setting +\ifdeluxestar +\gdef\two{#2}\gdef\checkh{h} +\ifx\two\checkh\onecolumngrid\fi +\begin{table*}[#2]\hsize=\textwidth\else + \begin{table}[#2]\fi +\noindent\setbox\splitbox=\vtop\bgroup% +\currtabletypesize + \vspace*{\abovedeluxetableskip} +%% +\def\startdata##1\enddata{% +\currtabletypesize +\setbox0=\hbox{ +\begin{tabular}{#1} +\pt@head +##1\end{tabular}} +\expandafter\ifx\csname @tablecaption\endcsname\empty\else +%% +\noindent\hbox +to\hsize{\hss\vtop{\hsize=\wd0 +\caption{\@tablecaption}}\hss}\vskip3pt\fi + +%% not here +\global\setbox3\hbox{% +\begin{tabular}{#1}% +\hline\hline\noalign{\vskip-9pt}% +\pt@head% +##1\crcr% added october 2017 +\omit\\\omit\\\hline\end{tabular}} + +%\noindent\hskip-1.25em %% kludge! but seems necessary +\hbox to\hsize{\hss\copy3\hss} +\global\setbox4\vtop\bgroup\ifdeluxestar\hsize=\textwidth\else\hsize=\wd0\fi\leftskip6pt\parindent-6pt +}} + +\def\zdeluxetable#1{\global\breaktabtrue +\let\colnumbers\deluxecolnumbers +\global\deluxedecimalsfalse +\let\decimals\deluxedecimals +\let\decimalcolnumbers\deluxedecimalcolnumbers +\let\tablehead\ztablehead +\gdef\tabfullpreamble{#1}%<<== needed +\def\endtabular{\endarray +\global\let\zdoit\relax +\global\let\tdoit\relax +\global\Dfalse} +\global\breaktabtrue +\global\colnumsused=0 +\global\colcount=0 +%% +%%%%%%%%%%%% + \lineskiplimit=\z@ % restore default setting +\ifdeluxestar +\begin{table*}\hsize=\textwidth\else + \begin{table}\fi +\noindent\setbox\splitbox=\vtop\bgroup% +\currtabletypesize + \vspace*{\abovedeluxetableskip} +%% +\def\startdata##1\enddata{% +\currtabletypesize +\setbox0=\hbox{\colnumbersonfalse +\begin{tabular}{#1} +\pt@head %% +##1\end{tabular}}% not here +\expandafter\ifx\csname @tablecaption\endcsname\empty\else +\noindent\hbox +to\hsize{\hss\vtop{\hsize=\wd0 +\caption{\@tablecaption}}\hss}\vskip3pt\fi +\global\setbox3\hbox{% +\begin{tabular}{#1}% +\hline\hline\noalign{\vskip-9pt}% +\pt@head% +##1\crcr%% added October 2017 +\omit\\\omit\\\hline\end{tabular}}%%<<== original +\vskip-\parskip +\noindent\hbox to\hsize{\hss\copy3\hss} +\global\setbox4\vtop\bgroup\hsize=\wd0\relax +\leftskip6pt\parindent-6pt +}} + + +%% go to \end{deluxetable}, after longdeluxetable + + + +%%@@@@ + +%% Variation on definition found in revtex4-1.cls +\def\LT@start@new{% + \let\LT@start\endgraf + \endgraf + \markthr@@{}% + \LT@pre + \@ifvoid\LT@firsthead{\LT@top}{\hbox{\ifdim\movetableright>0pt\relax\hskip\movetableright\fi\box\LT@firsthead} +\nobreak}% + \mark@envir{longtable}% +}% + +%%% +\newbox\longtablebox +\def\longdeluxetable#1{ +\global\rotateonfalse +\let\colnumbers\deluxecolnumbers +\global\deluxedecimalsfalse +\let\decimals\deluxedecimals +\let\decimalcolnumbers\deluxedecimalcolnumbers +\let\tablehead\ztablehead +\gdef\tabfullpreamble{#1}%<<== needed +\def\endtabular{\endarray +\global\let\zdoit\relax +\global\let\tdoit\relax +\global\Dfalse} +\global\colnumsused=0 +\global\colcount=0 +%% +%%%%%%%%%%%% + \lineskiplimit=\z@ % restore default setting +\let\enddeluxetable\endlongdeluxetable + \vspace*{\abovedeluxetableskip} +%% +\def\startdata##1\enddata{% +\global\setbox\longtablebox=\hbox{\currtabletypesize +\tabcolsep=3pt +\begin{tabular}{#1} +\pt@head +##1\end{tabular}} +%%% +\bgroup\centering +\def\table@hook{\currtabletypesize} + \LTcapwidth=\wd\longtablebox +%% march 2019, added [c] and these terms: +\ifcenterwidetable\global\centerwidetablefalse + \def\LT@LR@c{\LTleft=0pt minus1fill + \let\LTright\LTleft}% +\else +%% default, will center table that is narrower than text width + \def\LT@LR@c{\LTleft=0pt plus1fill + \LTright\LTleft}% +\fi +%% +% +\begin{longtable}[c]{#1}%% +\ifdim\movetableright>0pt + \noalign{\ifdim\movetableright>0pt + \global\LTleft=\movetableright + \fi} +% + \noalign{\hbox to \wd\longtablebox{ + \vtop{\hsize=.8\wd\longtablebox + \advance\baselineskip4pt + \raggedright + {\bf \fnum@table}.\vrule depth 6pt width0pt\ + \@tablecaption}\hss}\vskip-3pt }\\ + \hline + \hline\noalign{\vskip-9pt} + \pt@head% +\else +\caption{\hsize=\wd\longtablebox +\advance\baselineskip2pt +\@tablecaption}\\ % +\hline\hline\noalign{\vskip-9pt}% prob ok +\pt@head% +\fi +\endfirsthead + +\noalign{\centerline{\small +\hskip\movetableright{\bf \fnum@table}\ \it(continued)}\vskip6pt} +\hline\hline +\noalign{\vskip-12pt} +\pt@head% +\endhead + +\hline +\multicolumn{\totalcolumns}{c}{\vrule height 24pt width0pt\small\it +\fnum@table\ +continued \if@two@col\else on next page\fi}\\ +\endfoot + +\hline%\nobreak +\endlastfoot +##1 +\end{longtable} +\vglue-\LTpost +\vskip-6pt +\egroup +\global\setbox4=\vtop\bgroup +\ifdim\wd\longtablebox>\textwidth +\hsize=\textwidth +\else +\hsize=\wd\longtablebox\fi +\leftskip=6pt +\parindent=-6pt +\currtabletypesize +\global\startlongtablefalse +\global\movetableright=0pt +}% end data, endlongtable +} + +\def\endlongdeluxetable{ +%% +\vrule depth 6pt width 0pt +\vskip1sp +\egroup +\ifdim\dp4>6pt +\vglue-6pt +\vbox{\hbox to \columnwidth{\hfill +\vtop{\hsize\wd\longtablebox +\leftskip=6pt\parindent-6pt +\copy4 +}\hfill}%% +} +\fi +\vglue\ht4 +\global\colnumbersonfalse +\global\deluxedecimalsfalse +\global\rotateonfalse +%% +\relax\null%% \null is an empty hbox. +%% This keeps final page(s) of startlongtable/deluxetable +%% from begin thrown away when at end of article. +% \global\advance\c@table-1\relax +%% +% +%% march 2019 +\ifreturntotwocol\global\returntotwocolfalse +\twocolumngrid\fi +%% May 2020 +\ifappendixon +\if@two@col@app +\twocolumngrid +\else +\onecolumngrid\fi\fi +\null +}%% + + +%% bbb +%% \end{deluxetable}: +\def\enddeluxetable{% +\egroup%end box 4 +\ifdim\dp4>6pt +\hbox to\hsize{\hss\copy4\hss} +\fi +\egroup% end splitbox +\centering +\ifrotateon\global\rotateonfalse +\rotatebox{90}{\hbox to\textheight{\hfill\vbox{ +\unvbox\splitbox +\vspace*{\belowdeluxetableskip}}\hfill}} +\else +\centering\unvbox\splitbox +\vspace*{\belowdeluxetableskip} +\vspace*{24pt} +\fi +\ifdeluxestar\end{table*}\global\deluxestarfalse +\if@two@col +\twocolumngrid\hsize=\columnwidth\fi%% check this!! +\else +\end{table}\fi +\null +% added june 2020 +\gdef\colnumbers{\saveplaincolnumbers} +\global\breaktabfalse +\global\deluxefalse +\global\colnumbersonfalse +\global\deluxedecimalsfalse +\global\rotateonfalse +\startlongtablefalse +\global\movetableright=0pt +%\global\floatfalse +%\global\advance\c@table by -1\relax +%% check this!! +} + +%%@@@ ??? + +\newbox\splitbox +\newif\ifdeluxe +\def\splitdeluxetable{ +%% Mar 30, 2019, to make label outside of \caption work correctly +{\advance\c@table by 1 +\xdef\@currentlabel{\thetable}} +\global\deluxetrue\catcode`\&=\active +\catcode`\$=\active +\xsplitdeluxetable} + +\def\xsplitdeluxetable#1{ +\global\breaktabtrue +\let\colnumbers\deluxecolnumbers +\let\decimals\deluxedecimals +\global\deluxedecimalsfalse +\let\decimalcolnumbers\deluxedecimalcolnumbers +\let\tablehead\xtablehead +\gdef\tabfullpreamble{#1} +\def\endtabular{\endarray +\global\let\zdoit\relax +\global\let\tdoit\relax +\global\Dfalse} +%%% modification of emulateapj \deluxetable %%%% +\setbox0=\hbox{\def\firstarg{#1}\expandafter\lookforD\firstarg} +\gdef\temppreamble{#1\relax} +\PartsOfTable=0 +\def\tempfullpreamble{#1BB} +\setbox0=\hbox{\expandafter\checkforB\tempfullpreamble} +%% Now PartsOfTable is either =2 or 3 +%% +\gdef\one{#1Z} +\global\colnumsused=0 +\global\breaktabtrue +\global\colcount=0 +%% +\ifnum\PartsOfTable=3 +\let\multicolumn\threebreakmulticolumn +\else +\let\multicolumn\breakmulticolumn +\fi +%%%%%%%%%%%% + \lineskiplimit=\z@ % restore default setting + \gdef\tblnote@list{} + \gdef\tblref@list{} +\ifsplitstar + \begin{table*}\else + \begin{table}\fi +\noindent\setbox\splitbox=\vtop\bgroup% +\currtabletypesize + \vspace*{\abovedeluxetableskip} +\let\startdata\xstartdata} +%% \end{splitdeluxetable}: + +\newdimen\movetabledown + +\def\endsplitdeluxetable{\vskip1sp\egroup%% end box with tablenotes +\hbox to \hsize{\hss\copy4\hss} +\egroup +\vskip1pt +\ifrotateon\global\rotateonfalse +\vskip\movetabledown\rotatebox{90}{\vbox{\noindent\unvbox\splitbox % +\vspace*{\belowdeluxetableskip} +}}\global\movetabledown=0pt\else +\noindent\unvbox\splitbox +\vspace*{\belowdeluxetableskip} +\fi +\ifsplitstar +\end{table*} +\else +\end{table}\fi +\gdef\colnumbers{\saveplaincolnumbers} +\tabletypesize{\small} +\global\breaktabfalse +\global\deluxefalse +\global\splitstarfalse +\global\colnumbersonfalse +\global\deluxedecimalsfalse +} + + +\newif\ifsplitstar +\expandafter\def\csname splitdeluxetable*\endcsname{\global\splitstartrue\splitdeluxetable} +\expandafter\def\csname endsplitdeluxetable*\endcsname{\endsplitdeluxetable\global\splitstarfalse +\global\colnumbersonfalse +\global\deluxedecimalsfalse +} + +\newdimen\maxtablewidth + +\gdef\NoTableCaption{\global\@table@not@headedtrue} + +%% For splitdeluxetable + +%%% ====================================================== %%% +\gdef\dbreaktabular{\catcode`\&=\active +\let&\CheckNumberAndSwitch\xdbreaktabular} + +\long\gdef\xdbreaktabular#1{%% #1=contents of table +{\global\maxtablewidth=0pt +\let&\CheckNumberAndSwitch +\let$\savedollar +\global\colnumsused=0 +%% +\global\dbreaktabtrue +\global\colcount=0 +%% +\ifnum\PartsOfTable=3 +\let\multicolumn\threebreakmulticolumn +\else +\let\multicolumn\breakmulticolumn +\fi +%% +\ifnum\PartsOfTable=3 +\expandafter\catchfirstpreamble\one +\expandafter\catchsecondofthreepreamble\one +\expandafter\catchthirdpreamble\one +\makefirstdummycolumns +\makeseconddummycolumns +\makethirddummycolumns +\else %% PartsOfTable=2 +\ifnum\PartsOfTable=2 +\expandafter\catchfirstpreamble\one +\expandafter\catchsecondpreamble\one +\makefirstdummycolumns +\makeseconddummycolumns +\fi\fi +%%% +\global\columncount=0 +\ifnum\PartsOfTable=3 +%% For table divided into three parts +\firstboxtrue\secondboxfalse\thirdboxfalse +\setbox\firsttablebox=\hbox{% +\begin{tabular}{AFE} +\ifx\csname pt@head\endcsname\relax\else +\pt@head\fi#1\crcr\end{tabular}} +\global\maxtablewidth=\wd\firsttablebox + +\noindent\hbox to \hsize{\hss\unhbox\firsttablebox\hss} +\vskip6pt +\hrule +\vskip6pt +\global\columncount=0 +\firstboxfalse\secondboxtrue\thirdboxfalse +\ifcolnumberson% +\setbox\secondtablebox=\hbox{% +\let\savecolnumbers\xcolnumbers% +\notfirsttrue% +\begin{tabular}{fZE} %fZE !!! +\ifx\csname pt@head\endcsname\relax\else% +\pt@head\fi#1\crcr\end{tabular}} +\else +%% +\setbox\secondtablebox=\hbox{% +\begin{tabular}{fZE}% +\ifx\csname pt@head\endcsname\relax\else% +\pt@head\fi\\ [-14pt]% +#1\crcr% +\end{tabular}} +\fi +\ifdim\wd\secondtablebox>\maxtablewidth +\global\maxtablewidth\wd\secondtablebox\fi + +\noindent\hbox to \hsize{\hss\unhbox\secondtablebox\hss} +%% +\vskip6pt +\hrule +\vskip6pt +\firstboxfalse\secondboxfalse\thirdboxtrue +\global\columncount=0 +\ifcolnumberson +\notfirsttrue +\setbox\thirdtablebox=\hbox{ +\let\savecolnumbers\xcolnumbers +\notfirsttrue +\begin{tabular}{fFz} +\ifx\csname pt@head\endcsname\relax\else +\pt@head\fi#1\crcr\end{tabular}} +\else +\setbox\thirdtablebox=\hbox{ +\begin{tabular}{fFz} +\ifx\csname pt@head\endcsname\relax\else +\pt@head\fi\\[-14pt] +#1 +\end{tabular}} +\fi +\ifdim\wd\thirdtablebox>\maxtablewidth +\global\maxtablewidth\wd\thirdtablebox\fi + +\noindent\hbox to \hsize{\hss\unhbox\thirdtablebox\hss} +\vskip6pt +\hrule +\else +%% Original for table divided into two parts +\global\columncount=0 +\secondboxfalse +\setbox\firsttablebox=\hbox{% +\begin{tabular}{AF} +\ifx\csname pt@head\endcsname\relax\else +\pt@head\fi% +#1\end{tabular}} +\global\maxtablewidth=\wd\firsttablebox +\hbox to \hsize{\hss\unhbox\firsttablebox\hss} +\vskip6pt +\hrule +\vskip6pt +\global\columncount=0 +\secondboxtrue +\ifcolnumberson +\setbox\secondtablebox=\hbox{% +\let\savecolnumbers\xcolnumbers +\notfirsttrue +\begin{tabular}{fZ}%% +\ifx\csname pt@head\endcsname\relax\else% +\pt@head\fi#1\crcr%%= tablecontents +\end{tabular}}% +\else +\setbox\secondtablebox=\hbox{% +\begin{tabular}{fZ}%% was 12 +\ifx\csname pt@head\endcsname\relax\else% +\pt@head\fi\\[-14pt]% +#1%%= tablecontents +\end{tabular}}\fi +\ifdim\wd\secondtablebox>\maxtablewidth +\global\maxtablewidth\wd\secondtablebox\fi + +\noindent\hbox to \hsize{\hss\unhbox\secondtablebox\hss} +\vskip6pt +\hrule +\secondboxtrue +%% +%% end of conditional testing for 2 or 3 part table: +\fi +%% +\global\dbreaktabfalse}} +%%% ====================================================== %%% + +\newif\ifnotfirst +%% @@@@ +%% xstartdata, modified from \startdata in emulateapj, for splitdeluxetable +\gdef\xstartdata#1\enddata{\def\tablecontents{% +\ifcolnumberson% +\\\savecolnumbers\\[2pt]\fi% this is for top level split +\ifdeluxedecimals\savedecimals\fi% +#1}% +\currtabletypesize% +\setbox2=\vtop{\dbreaktabular{\tablecontents}}% +% +\expandafter\ifx\csname @tablecaption\endcsname\empty\else +\noindent\hbox +to\hsize{\hss\vtop{\hsize=\maxtablewidth\caption{\@tablecaption}}\hss}\vskip3pt\fi +\dbreaktabular{\tablecontents\noalign{\global\let\zdoit\relax +\global\let\ddoit\relax}} +\parindent=0pt +\global\setbox4=\vtop\bgroup% egroup in enddeluxetable +\currtabletypesize +\ifsplitstar +\hsize=\textwidth\else\hsize=245.3pt\fi +\parindent=-6pt \leftskip=6pt +} + +\def\tablecomments#1{\vskip1pt{\small\vskip1sp\indent\vrule height 11pt depth 2pt +width 0pt\currtabletypesize{\sc Note}---{#1}\vskip1pt}} + +\def\tablenotetext#1#2{\vskip1pt{\currtabletypesize\vskip1pt\indent\vrule +height 11pt depth +2pt width0pt\relax$^{\hbox to 5pt{$#1$}}$#2\vskip1pt}} + +\def\tablerefs#1{{\small\vskip3pt\indent\vrule height 11pt depth 2pt +width 0pt\currtabletypesize{\bf References}---{#1}\vskip1sp}} + +\let\tablereferences\tablerefs + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% 5. Simple entry decimal numbers + +%% extra unused args are to get rid of unnecessary commands revtex puts in +\gdef\lookfordecimal#1#2#3#4.#5 {\gdef\xone{{\let$\relax\savedollar#4\savedollar}} +\gdef\xtwo{#5}\ifx\xtwo\empty\else\gdef\xtwo{{\let$\relax\savedollar#5\savedollar}}\fi} + +%% D +\def\newdoit{\setbox0=\hbox\bgroup\zdoit} +\def\endnewdoit{\egroup\unhbox0} + +\long\gdef\zdoit#1 {\let$\relax +\def\bothcols{#1 }% +\setbox0=\hbox{\let$\relax\expandafter\lookfordecimal\bothcols{}{}{}{}.{} }% +\xdoit} + +\global\let\savezdoit\zdoit +\let\zdoit\relax + +\gdef\xdoit{\relax\hskip\tabcolsep\relax\xone&\tabskip=0pt% +\ifx\xtwo\empty\let\go\relax\else.\def\go{\xtwo}\fi\go} + +%% d +\def\xnewdoit{\setbox0=\hbox\bgroup\ddoit} +\def\xendnewdoit{\egroup} + +\long\gdef\ddoit#1#2#3{\xxdoit} +\let\saveddoit\ddoit +\let\ddoit\relax + +%% to delete all D material: + +\gdef\xxdoit{&} + +\newcolumntype{D}{>\newdoit r<{\endnewdoit} @{}l}%% +\newcolumntype{d}{>\xnewdoit h<{\xendnewdoit} @{}h} %% + +\newdimen\savetabskip +\gdef\decimals{\noalign{\global\savetabskip\tabskip +\tabskip=0pt +\global\let\extracolsep\relax +\global\let\ddoit\saveddoit +\global\let\zdoit\savezdoit +}} + +\let\savedecimals\decimals + +%% to allow \decimals to be used before \startdata: +\newif\ifdeluxedecimals +\def\deluxedecimals{\global\deluxedecimalstrue} + +%%%%%%%%% +%% This needed to be redefined so that \colhead in \tablehead would span both parts +%% of decimal numbers. + +%% in case there isn't a table head +\let\pt@head\relax + +%% for splitdeluxetable +\def\xtablehead{\catcode`\&=\active% +\catcode`\$=\active% +\xxtablehead} + +%% +\def\xxtablehead#1{% +\let&\CheckNumberAndSwitch% +\gdef\pt@head{% +\hline\hline% +\multicolumn1c{\vrule height 12pt width0pt\relax\tempcounter=0 +\expandafter\getDs\tabfullpreamble\relax +\global\colcount=0 +\global\colheadcount=0}% +\\ +\iftwelvepoint% + \ifpreprint% + \iflongrotateon\else\noalign{\vskip-6.5pt}\fi% + \else% + \ifpreprinttwo% + \iflongrotateon\else\noalign{\vskip-6.5pt}\fi% + \else% + \ifmanu% + \iflongrotateon\noalign{\vskip-8pt}\else\noalign{\vskip-17pt}\fi% + \else% + \ifmodern\iflongrotateon\else\noalign{\vskip-9pt}\fi% + \else% + \fi%% end ifmodern + \fi%% end ifmanu + \fi%% end ifpreprinttwo + \fi%% end ifpreprint +\else% +%% not twelvepoint + \iftwocolstyle% + \iflongrotateon\else\noalign{\vskip-5pt}\fi% + \else% + \ifonecolstyle% default + \iflongrotateon\noalign{\vskip2pt}\else\noalign{\vskip-4.5pt}\fi% + \fi% end ifonecol + \fi%endiftwocolstyle +\fi%end iftwelvepoint +#1\ifcolnumberson% +\ifnotfirst\\[-22pt]\fi +\else\\\hline\\[-8pt]\fi% space below hline for 2nd and 3rd part of split table +}% +% +} + +\def\ztablehead{\catcode`\&=\active% +\catcode`\$=\active% +\zztablehead} + +\def\zztablehead#1{\let&\CheckNumberAndSwitch% +\gdef\pt@head{% +%% this is needed: +\multicolumn1c{\vrule height12pt width0pt\relax\expandafter\getDs\tabfullpreamble\relax +\global\tempcounter=0 +\global\colcount=0 +\global\colheadcount=0}\\ +\iftwelvepoint% + \ifpreprint% + \iflongrotateon\else\noalign{\vskip-6.5pt}\fi% + \else% + \ifpreprinttwo% + \iflongrotateon\else\noalign{\vskip-6.5pt}\fi% + \else% + \ifmanu% + \iflongrotateon\noalign{\vskip-8pt}\else\noalign{\vskip-17pt}\fi% + \else% + \ifmodern \iflongrotateon\else\noalign{\vskip-5pt}\fi% + \else% + \fi%% end ifmodern + \fi%% end ifmanu + \fi%% end ifpreprinttwo + \fi%% end ifpreprint +\else% +%% not twelvepoint + \iftwocolstyle% + \iflongrotateon\else\noalign{\vskip-5pt}\fi% + \else% + \ifonecolstyle% default + \iflongrotateon\noalign{\vskip2pt}\else\noalign{\vskip-4.5pt}\fi% + \fi% end ifonecol + \fi%endiftwocolstyle +\fi%end iftwelvepoint +#1\unskip% +\ifcolnumberson\\[6pt] +\savecolnumbers\vrule height 11pt depth 4pt width 0pt\relax% +\\\ifmanu\noalign{\vskip-15pt}\fi% +\ifdeluxedecimals\\[-14pt]% +\savedecimals\fi% +\else \vrule depth 6pt +width0pt\\\ifdeluxedecimals\savedecimals\fi\hline\fi% +}} + + +\newcount\tempcounter + +\gdef\getDs#1{\let&\CheckNumberAndSwitch +\def\lookforD{#1}% +\ifx\lookforD\xD% +\expandafter\gdef\csname col\the\tempcounter\endcsname{2}\else +\expandafter\gdef\csname col\the\tempcounter\endcsname{1}\fi +\global\advance\tempcounter by 1 +\futurelet\next\checkingpreamble} + +\gdef\checkingpreamble{\ifx\next\relax +\let\go\relax\else\let\go\getDs\fi\go} + +%%% Something like this could be used to automate the width of colheads in the tablehead, +%% making those that match the D in preamble are multicolumn2c instead of +%% multicolumn 1c. +\newcount\colheadcount +\newcommand\xcolhead[1]{\multicolumn{\expandafter\ifx\csname +col\the\colheadcount\endcsname\relax 1\else\expandafter% +\csname col\the\colheadcount\endcsname\fi}{c}{\vrule depth 4pt +width0pt\relax#1\relax\global\advance\colheadcount +by 1\relax}\ignorespaces}% +% + +%% +\extrarowheight=2pt +%% from revtex4-1, additions on top +%% fix for \usepackage{amsmath} and +%% any matrix environment +\def\matrixpreamble{*\c@MaxMatrixCols c} +%% this causes problem, must be fixed! +%\let\save@array@array@new\@array@array@new +\def\@array@array@new[#1]#2{% +\ifbreaktab +\else +%%% added so that we can use \colnumbers in any tabular environment +%%% and avoid error messages for breaktabular +\def\catchpreamble{#2\relax} +\gdef\tabfullpreamble{#2\relax} +{\colcount=0 +%% important fix, makes it possible to use amsmath and matrices. +\def\two{#2} +\ifx\matrixpreamble\two +\else +\expandafter\countcols\catchpreamble +\global\totalcolumns=\colcount\fi} +\fi +%%% end of additions + \@tempdima\ht\strutbox + \advance\@tempdima by\extrarowheight + \setbox\@arstrutbox\hbox{% + \vrule \@height\arraystretch\@tempdima + \@depth \arraystretch\dp\strutbox + \@width \z@ + }% + \begingroup + \@mkpream{#2}% + \xdef\@preamble{\@preamble}% + \endgroup + \prepdef\@preamble{% + \tabskip\tabmid@skip + \@arstrut + }% + \appdef\@preamble{% + \tabskip\tabright@skip + \cr + \array@row@pre + }% + \@arrayleft + \@nameuse{@array@align@#1}% + \m@th + \let\\\new@arraycr %<<== defined above, original plus reset counters + \let\tabularnewline\\% + \let\par\@empty + \let\@sharp##% + \set@typeset@protect + \lineskip\z@\baselineskip\z@ + \tabskip\tableft@skip + \everycr{}% + \expandafter\halign\expandafter\@halignto\expandafter\bgroup\@preamble +}% + +%% \rotate +\newif\ifrotateon +\def\rotate{\global\floattrue\iffloat\global\let\go\relax\global\rotateontrue\else +\global\rotateonfalse +\let\go\relax +%\def\go{\vskip48pt\huge +%{\tt \string\floattable\space must precede table using +%\string\rotate !!}} +\fi\go} + +\def\colnumbers{\plaincolnumbers} + +%% add 6pt of space between table and following text: +\let\saveendtable\endtable +\def\endtable{\vskip6pt\saveendtable} +\expandafter \let \csname endtable*\endcsname = \endtable +%% + + +%%% \movetabledown works +\newbox\rotatetablebox +\def\rotatetable{% +\clearpage +\global\startlongtabletrue\setbox\rotatetablebox=\vbox\bgroup +} + +\def\endrotatetable{\egroup +\vglue\movetabledown +\hbox to +\textwidth{\hss\rotatebox{90}{\hbox{\box\rotatetablebox}}\hss} +\global\movetabledown=0pt\relax +\global\startlongtablefalse +} + +%%% \movetabledown works +\expandafter\def\csname rotatetable*\endcsname{% +\clearpage +\global\startlongtabletrue\setbox\rotatetablebox=\vbox to +\textwidth\bgroup\vfill} + +\expandafter\def\csname endrotatetable*\endcsname{\vfill\egroup +\vbox to \textheight{\vfill +\vglue\movetabledown +\hbox to +\textwidth{\hss\rotatebox{90}{\box\rotatetablebox}\hss}\global\movetabledown=0pt\relax +\vfill} +\clearpage +\if@two@col +\twocolumngrid +\global\startlongtablefalse +} + +% +%%% \movetabledown works +\newif\iflongrotateon +\def\longrotatetable{% +\global\longrotateontrue + \if@two@col\onecolumngrid\clearpage + \fi +\clearpage + \clearpage + \begingroup +\expandafter\def\csname deluxetable*\endcsname{\deluxetable} +\expandafter\def\csname enddeluxetable*\endcsname{\enddeluxetable} +\global\floatfalse +\global\startlongtabletrue +\def\LS@rot{% + \setbox\@outputbox\vbox{\vskip\movetabledown\hbox{\rotatebox{90}{\box\@outputbox}}}} + +\let\LS@makecol=\@makecol +\let\LS@makefcolumn=\@makefcolumn + + \vsize=\textwidth + \hsize=\textheight + \linewidth=\hsize + \columnwidth=\hsize + \@colroom=\vsize + \textheight=\vsize + \@colht=\vsize + \def\@makecol{\LS@makecol\LS@rot}% + \def\@makefcolumn##1{\LS@makefcolumn{##1}\LS@rot}} + +\def\endlongrotatetable{% +\onecolumngrid %% ?? +\clearpage + \ifGin@pdftex + \pdfpageattr{/Rotate 90} + \fi + \clearpage + \endgroup + \if@two@col\twocolumngrid\fi +\clearpage +\global\longrotateonfalse +\global\movetabledown=0pt + \global\@colht=\textheight + \global\vsize=\textheight + \global\@colroom=\textheight} + +\newif\ifGin@pdftex +\Gin@pdftexfalse +\DeclareOption{pdftex}{% + \PassOptionsToPackage\CurrentOption{graphicx} + \Gin@pdftextrue +} + +\DeclareOption*{\PassOptionsToPackage\CurrentOption{graphicx}} +\ProcessOptions + +%% set &, $ catcode back to normal: + +\catcode`&=4 +\catcode`$=3 + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% end table tools +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Gridlines for positioning multiple illustrations in +%% one figure environment. + +\def\gridline#1{\vskip6pt\hbox to\hsize{#1}\vskip6pt} + +\def\boxedfig#1#2#3{\hfill\fbox{\vbox{\parskip=0pt\relax +\hsize=#2 +\includegraphics[width=#2]{#1}\vskip2pt\vtop{\hsize=#2 +\centerline{#3}}}}\hfill} + +\def\fig#1#2#3{\hfill\vbox{\parskip=0pt\hsize=#2 +\includegraphics[width=#2]{#1}\vskip2pt\vtop{\centering +\footnotesize +\hsize=#2 +#3\vskip1pt +}}\hfill} + +\def\leftfig#1#2#3{\vbox{\parskip=0pt\relax\hsize=#2 +\includegraphics[width=#2]{#1}\vskip2pt\vtop{\hsize=#2 +\centering +#3\vskip1sp\vskip1sp}}\hfill} + +\def\rightfig#1#2#3{\hfill\vbox{\parskip=0pt\relax\hsize=#2 +\includegraphics[width=#2]{#1}\vskip2pt\vtop{\hsize=#2 +\centering#3\vskip1sp}}} + +\def\rotatefig#1#2#3#4{\hfill\vbox{\centering\parskip=0pt\hsize=#3 +\includegraphics[width=#3,angle=#1]{#2}\vskip2pt\vtop{\centering +\footnotesize +\hsize=#3 +#4\vskip1pt +}}\hfill} + +%%%%%%%%%% End Grid line Macros %%%%%%%%%% + +%%%%%%%%%% Color Editing Macros %%%%%%%%%% +%% \turnoffedit or \turnoffedits +%% will prevent all \edit{text}, all +%% \collaborationcomment{text}, and all +%% \authorcomment{text} from producing any text. + +\newif\ifturnoffedit +\def\turnoffedit{\global\turnoffedittrue} +\def\turnoffedits{\global\turnoffedittrue} +\let\turnoffediting\turnoffedits + +\newif\ifturnoffone +\newif\ifturnofftwo +\newif\ifturnoffthree + +%% \turnoffeditone to only turn off only \edit1, \collaborationcomment1 and \authorcomment1 : +\def\turnoffeditone{\turnoffonetrue} + + +%% \turnoffedittwo to only turn off only \edit2, \collaborationcomment2 and \authorcomment2 : +\def\turnoffedittwo{\turnofftwotrue} + + +%% \turnoffeditthree to only turn off only \edit3, \collaborationcomment3 and \authorcomment3 : +\def\turnoffeditthree{\turnoffthreetrue} + + +%% Other choices can be made, but this should be +%% standardized, so didn't make an user interface +%% to change the colors easily. + +\expandafter\def\csname editcolor1\endcsname{black}% was magenta +\expandafter\def\csname editcolor2\endcsname{black}% was blue +\expandafter\def\csname editcolor3\endcsname{black}% was violet + +\let\newgo\relax +\newcount\colorcount + +\newcount\editnum +\def\edit#1#2{\ifcase#1\or\ifturnoffone% +\unskip% +\else% +\texorpdfstring{{\bf#2}}{#2}\fi\or% +\ifturnofftwo% +\unskip% +\else\texorpdfstring{{\bfseries\itshape#2}}{#2}\fi% +\or% +\ifturnoffthree\unskip\else% +\texorpdfstring{{\bfseries\underline{#2}}}{#2}\fi\fi} + +\def\collaborationcomment#1#2{{\colorcount=#1 +\ifturnoffedit\let\go\ignorespaces\else% +\let\go\relax% +\color{\csname editcolor\the\colorcount\endcsname} +\ifnum\colorcount=1{\ifturnoffone\else\bf (Collaboration~note: #2)\ \fi}\else +\ifnum\colorcount=2{\ifturnofftwo\else\it (Collaboration~note: #2)\ \fi}\else +\ifnum\colorcount=3{\ifturnoffthree\else (Collaboration~note: #2)\ \fi}\fi\fi\fi\fi% +\go}} + +\def\authorcomment#1#2{{\colorcount=#1 +\ifturnoffedit\let\go\ignorespaces\else% +\let\go\relax% +\color{\csname editcolor\the\colorcount\endcsname} +\ifnum\colorcount=1{\ifturnoffone\else\bf (Author~note 1: #2)\ \fi}\else +\ifnum\colorcount=2{\ifturnofftwo\else\it (Author~note 2: #2)\ \fi}\else +\ifnum\colorcount=3{\ifturnoffthree\else (Author~note 3: #2)\ \fi}\fi\fi\fi\fi% +\go}} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%% Draft watermark + +\definecolor{ltgray}{gray}{.9}% .89 +\font\bighelv=phvr at 2in % +\def\setwatermarkfontsize#1{\font\bighelv=phvr at #1} + +\def\watermark#1{\def\thewatermark{\hbox to\textwidth{\vtop to +1.1\textheight{\vss +\hskip24pt\rotatebox{60}{\hbox{\bighelv \color{ltgray} +\uppercase{#1}}}\vss}}\hss}} +\let\thewatermark\empty + +%% Used in titlepage definition, as \pagestyle{titlepage} +\def\ps@titlepage{% + \let\@mkboth\@gobbletwo +\def\@oddhead{\ifx\thewatermark\empty\hfill\else +\hbox to \textwidth{\rlap{\thewatermark}\hfill}\fi} +\let\@oddfoot\@empty +\let\@evenhead\@empty\let\@evenfoot\@empty} + +% end of watermark definitions +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +\newcommand*\submitjournal[1] +{\def\@submitted{Submitted to #1}}% + +%% this one is used &&& +\def\titleblock@produce{% + \begingroup + \ltx@footnote@pop + \def\@mpfn{mpfootnote}% + \def\thempfn{\thempfootnote}% + \c@mpfootnote\z@ + \let\@makefnmark\frontmatter@makefnmark + \frontmatter@setup + \thispagestyle{titlepage}\label{FirstPage}% +\ifmodern\leftskip=0pt\rightskip\leftskip\fi + \frontmatter@title@produce + \groupauthors@sw{% +\frontmatter@author@produce@group + }{% + \frontmatter@author@produce@script + }% + \frontmatter@RRAPformat{% +\vskip12pt + \expandafter\produce@RRAP\expandafter{\@date}% + \expandafter\produce@RRAP\expandafter{\@received}% + \expandafter\produce@RRAP\expandafter{\@revised}% + \expandafter\produce@RRAP\expandafter{\@accepted}% + \expandafter\produce@RRAP\expandafter{\@published}% + }% +\expandafter\ifx\csname @submitted\endcsname\relax\else +\vskip6pt +\expandafter\produce@RRAP\expandafter{\centerline{\@submitted\hbox +to 20pt{\hfill}}\vskip12pt}% +\fi + \frontmatter@abstract@produce + \@ifx@empty\@pacs{}{% + \@pacs@produce\@pacs + }% + \@ifx@empty\@keywords{}{% + \@keywords@produce\@keywords + }% + \par + \frontmatter@finalspace +\endgroup% +}% + + +% needed?? +\gdef\specialbibitem#1[#2]#3#4{ +{\tt\string\bibitem}[#2]{\tt\string{\string}} +#4} + + + +%%%%%%%%%%%%%%%%%%%%%%%%% +%% Track Changes +%% Amy Hendrickson, Nov 2015 +%% Change Jan 2016, to allow list of changes +%% to give line and page numbers for more than one entry on the same line. +%% Change Feb 2016, to allow optional argument for time/date, and/or editor initials, etc. + + +\providecolor{trackchange}{cmyk}{0,0,0,1} +\providecolor{explain}{cmyk}{0,0,0,1} + +\newif\ifsilent + +\newcount\refchangenumber +\def\added{\@ifnextchar[{\xadded}{\yadded}} + +\long\def\xadded[#1]#2{% +\iftrack {\global\advance\refchangenumber by 1\relax% +\vtop to 0pt{\vss +\hypertarget{link\the\refchangenumber}{} +\vskip14pt}% +\ifnumlines% +\ifabstract\else% +\xdef\doit{\noexpand\linelabel{\the\refchangenumber}}\doit\fi\else% +\xdef\doit{\noexpand\label{\the\refchangenumber}{}{}{}}\doit\fi}% +{\color{trackchange}\bf(Added: [#1] #2)}%% +\ifabstract\label{\the\refchangenumber}% +\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{\bf Added: [#1] +\textcolor{trackchange}\bf\relax{#2}\global\silenttrue}% +\else\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{\bf\relax Added: [#1] +\textcolor{trackchange}\bf\relax{\let\bibitem\specialbibitem #2}\global\silentfalse}\fi% +\else#2\fi} + + + +\long\def\yadded#1{% +\iftrack{\global\advance\refchangenumber by 1\relax% +\vtop to 0pt{\vss +\hypertarget{link\the\refchangenumber}{} +\vskip14pt}% +\ifnumlines\ifabstract\else% +\xdef\doit{\noexpand\linelabel{\the\refchangenumber}}\doit\fi\else% +\xdef\doit{\noexpand\label{\the\refchangenumber}{}{}{}}\doit% +\fi}% +{\color{trackchange}\bf(Added: #1)}%% +\ifabstract% +\label{\the\refchangenumber}% +\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{\bf Added: +\textcolor{trackchange}\bf\relax{#1}, +\global\silenttrue}\else +\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{\bf Added: +\textcolor{trackchange}{\bf\relax\let\bibitem\specialbibitem #1},% +\global\silentfalse}\fi% +\else#1\fi} + + + +\def\deleted{\@ifnextchar[{\xdeleted}{\ydeleted}} + +\long\def\xdeleted[#1]#2{\iftrack{\global\advance\refchangenumber by +1\relax% +\vtop to 0pt{\vss +\hypertarget{link\the\refchangenumber}{} +\vskip14pt}% +\ifnumlines\ifabstract\else% +\xdef\doit{\noexpand\linelabel{\the\refchangenumber}}\doit\fi% +\else% +\xdef\doit{\noexpand\label{\the\refchangenumber}}\doit\fi% +}% +{\color{trackchange}\bf% +\ifbib\let\sout\relax\fi% +(Deleted: [#1] \sout{#2}) +}% +\ifabstract\label{\the\refchangenumber}% +\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{Deleted: [#1] +{\color{trackchange}\bf% +\sout{#2}}\global\silenttrue}% +\else +\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{Deleted: [#1] +{\color{trackchange}% +\let\bibitem\specialbibitem% +\sout{#2} +}\global\silentfalse}\fi% +\fi} + +\long\def\ydeleted#1{\iftrack{\global\advance\refchangenumber by 1\relax% +\vtop to 0pt{\vss +\hypertarget{link\the\refchangenumber}{} +\vskip14pt}% +\ifnumlines\ifabstract\else% +\xdef\doit{\noexpand\linelabel{\the\refchangenumber}}\doit\fi% +\else% +\xdef\doit{\noexpand\label{\the\refchangenumber}{}{}{}}\doit% +\fi}% +%% +{\color{trackchange}\bf% +\ifbib\let\sout\relax\fi% +(Deleted: \sout{#1})}% +\ifabstract\label{\the\refchangenumber}% +\expandafter\gdef\csname changenum\the\refchangenumber\endcsname{Deleted: +{\color{trackchange}\bf +\sout{#1}}\global\silenttrue}% +\else +\expandafter\gdef\csname changenum\the\refchangenumber\endcsname{Deleted: +{\color{trackchange}\bf% +\sout{#1}}\global\silentfalse}\fi% +\fi} + + +\def\replaced{\@ifnextchar[{\xreplaced}{\yreplaced}} + +\long\def\xreplaced[#1]#2#3{% +\iftrack\global\advance\refchangenumber by 1\relax% +\vtop to 0pt{\vss +\hypertarget{link\the\refchangenumber}{} +\vskip14pt}% +\ifnumlines\ifabstract\else\xdef\doit{\noexpand\linelabel{\the\refchangenumber}}\doit\fi\else% +\xdef\doit{\noexpand\label{\the\refchangenumber}}\doit\fi% +{\ifbib\let\sout\relax\fi +\color{trackchange}\bf(Replaced: [#1] \sout{#2}}% +{\color{black}replaced with:} { +\color{trackchange}\bf\relax #3)}% +\ifabstract\label{\the\refchangenumber}% +\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{Replaced: [#1] +{\color{trackchange}\bf\relax\sout{#2}} {\color{black} replaced with:} +{\color{trackchange}\bf\relax#3}, \global\silenttrue}% +\else +\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{Replaced: [#1] +{\ifbib\let\sout\relax\fi +\color{trackchange}\bf\relax\sout{#2} +} {\color{black} replaced with:} +{\color{trackchange}\bf\relax#3}, \global\silentfalse}\fi% +\else#3\fi} + +\long\def\yreplaced#1#2{% +\iftrack\global\advance\refchangenumber by 1\relax% +\vtop to 0pt{\vss +\hypertarget{link\the\refchangenumber}{} +\vskip14pt}% +\ifnumlines\ifabstract\else\xdef\doit{\noexpand\linelabel{\the\refchangenumber}}\doit\fi\else% +\xdef\doit{\noexpand\label{\the\refchangenumber}}\doit\fi% +{\ifbib\let\sout\relax\fi +\color{trackchange}\bf\relax(Replaced: +\sout{#1} +}% +{\color{black}replaced with:} +{\color{trackchange}\bf\relax #2)}% +\ifabstract\label{\the\refchangenumber}% +\expandafter\gdef\csname changenum\the\refchangenumber\endcsname{Replaced: +{\color{trackchange}\bf\relax +\sout{#1}} {\color{black} replaced with:} +{\color{trackchange}\bf\relax#2},\global\silenttrue}% +\else +\expandafter\gdef\csname +changenum\the\refchangenumber\endcsname{Replaced: +{\ifbib\let\sout\relax\fi +\color{trackchange}\bf\relax\sout{#1} +} {\color{black} replaced with:} +{\let\bibitem\specialbibitem\color{trackchange}\bf\relax#2}, \global\silentfalse}\fi% +\else#2\fi} + +\def\explain{\@ifnextchar[{\xexplain}{\yexplain}} + +\def\xexplain[#1]#2{\iftrack\ {\bfseries\itshape\color{explain} [Explanation of change: +#2 (#1)]\ }\fi} + +\def\yexplain#1{\iftrack\ {\bfseries\itshape\color{explain} [Explanation of change: +#1]\ }\fi} + + +\newcount\listchangenum + +\def\listofchanges{ +\clearpage +\iftrack +\ifnum\refchangenumber>0 +\ifnumlines\nolinenumbers\fi +\vskip36pt +\hrule +\noindent{\vrule height 14pt width0pt depth 6pt\large\bf List of Changes} +\hrule +\vskip18pt +\nobreak +{\parskip=4pt \parindent=0pt +\loop +\global\silentfalse +\vskip-1pt\relax +\global\advance\listchangenum by 1\relax +\expandafter\ifx\csname changenum\the\listchangenum\endcsname\relax +\else +\csname changenum\the\listchangenum\endcsname\ +on page +%% can't get hyperlink to work correctly for page numbers, works but error messages. +\hyperlink{link\the\listchangenum}{\bf\pageref{\the\listchangenum}}% +\ifnumlines% +\ifsilent\global\silentfalse \else% +\setbox0=\hbox{\lineref{\the\listchangenum}}% +\ifdim\wd0<20pt% +, line\ +\hyperlink{link\the\listchangenum}{\lineref{\the\listchangenum}}% +\fi +\fi\fi.\relax +\repeat} +\fi\fi +\thispagestyle{empty} +} + + +\PassOptionsToPackage{normalem}{ulem} +\usepackage{ulem} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% From earlier version of AASTeX, for usefulness and +%% backward compatibility, with some requested additions + +\let\jnl@style=\rmfamily +\def\ref@jnl#1{{\jnl@style#1}}% + +%%% +\renewcommand\memsai{\ref@jnl{Mem.~Soc.~Astron.~Italiana}}% + % Mem. Societa Astronomica Italiana +%% longer version: +\newcommand\memsocai{Mem. Societ\`a Astronomica Italiana} +\newcommand\aspconf{Ast. Soc. of the Pac. Conference Series} + +\let\astap=\aap +\let\apjlett=\apjl +\let\apjsupp=\apjs +\let\applopt=\ao + +%%% More useful commands from Earlier version of Aastex: +\let\la=\lesssim % For Springer A&A compliance... +\let\ga=\gtrsim + +\let\farcm\farcm@mss +\let\farcs\farcs@mss + +\def\farcm@apj{% + \mbox{.\kern -0.7ex\raisebox{.9ex}{\scriptsize$\prime$}}% +}% + +\def\farcs@apj{% + \mbox{% + \kern 0.13ex.% + \kern -0.95ex\raisebox{.9ex}{\scriptsize$\prime\prime$}% + \kern -0.1ex% + }% +}% + +\def\chem@bnd#1{% + {% + \kern.1em\relax + \setbox\z@\hbox{M}% + \dimen@ii.8em\relax + \p@=.1em\relax + \dimen@.5\ht\z@\dimen@i-\dimen@ + \advance\dimen@1.5\p@\advance\dimen@i-1.0\p@ + #1% + \kern.1em\relax + }% + }% +\def\@sbnd{% + \advance\dimen@-1.5\p@\advance\dimen@i1.5\p@ + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + }% +\def\@dbnd{% + \advance\dimen@-0.5\p@\advance\dimen@i0.5\p@ + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + \advance\dimen@-1.5\p@\advance\dimen@i1.5\p@ + \hskip-\dimen@ii + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + }% +\def\@tbnd{% + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + \advance\dimen@-1.5\p@\advance\dimen@i1.5\p@ + \hskip-\dimen@ii + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + \advance\dimen@-1.5\p@\advance\dimen@i1.5\p@ + \hskip-\dimen@ii + \vrule\@height\dimen@\@depth\dimen@i\@width\dimen@ii\nobreak + }% + +\renewcommand\LaTeX{% + \leavevmode + L% + \raise.42ex\hbox{% + \count@=\the\fam + $\fam\count@\scriptstyle\kern-.3em A$% + }% + \kern-.15em\TeX +}% + +%% added Feb 2, 2016, redefining definition of \caption made with hyperref +%% package. Making \caption[] be the default, to prevent sending caption +%% text to listoftables or listoffigures, which we are not going to use +%% anyway. This change enables track changes commands to work in captions. +\def\xtable{table} +\def\caption{\numlinesfalse +\ifx\@captype\@undefined +\@latex@error {\noexpand \caption outside float}\@ehd +\expandafter \@gobble \else +\H@refstepcounter \@captype \let \Hy@tempa \@caption \@ifundefined +{float@caption}{} +{\expandafter \ifx \csname @float@c@\@captype\endcsname +\float@caption\let\Hy@tempa\Hy@float@caption\fi} +\expandafter\@firstofone\fi +{\@dblarg {\Hy@tempa \@captype}}[]} + +\def\@caption#1[#2]#3{{\small\rm\expandafter \ifx \csname if@capstart\expandafter \endcsname +\csname iftrue\endcsname \global \let \@currentHref \hc@currentHref \else \hyper@makecurrent {\@captype }\fi +\@ifundefined {NR@gettitle}{\def \@currentlabelname{\thesection\relax #2}} +{\NR@gettitle {#2}}\par +%\addcontentsline {\csname ext@#1\endcsname }{#1}{\protect \numberline {\csname the#1\endcsname }{\ignorespaces #2}} +\begingroup \@parboxrestore \if@minipage \@setminipage \fi \normalsize +\expandafter\ifx \csname if@capstart\expandafter \endcsname +\csname iftrue\endcsname \global \@capstartfalse +\@makecaption {\bf\csname fnum@#1\endcsname }{\ignorespaces #3} +\else \@makecaption {\bf\csname fnum@#1\endcsname }{\ignorespaces \ifHy@nesting +\expandafter \hyper@@anchor \expandafter {\@currentHref }{#3}\else +\Hy@raisedlink {\expandafter \hyper@@anchor \expandafter +{\@currentHref }{\relax }}{#3}\fi }\fi \par +\endgroup}} + +%% changed, March 23, 2019, took out \\ at end of definition: +\newcommand\tablebreak{\\[-11pt]\noalign{\break}} + +%% As suggested by Greg Schwarz, August Meunch, Feb 11 + +\def\dataset{\def\doi##1{https://doi.org/##1} +\@ifnextchar[{\ydataset}{\xdataset}} +\def\xdataset#1{\ydataset[]{#1}\let\doi\savedoi} +\def\ydataset[#1]#2{\def\one{#1}\ifx\one\empty +\href{#2}{[DATASET]}\else +\href{#2}{#1}\fi\let\doi\savedoi} + +%% this seems in the middle of nowhere... +\advance\columnsep6pt + +%%%%%%%%%% +%% macros to give hyperref link to authors when orcid numbers +%% are supplied with \author[0000-2345-3333-0023]{author name} + \def\lookforbracket{\ifx\next[\let\go\xauthor\else\let\go\yauthor\fi\go} + +\newcount\entriesinthiscollab +\newcount\allentries +\newif\ifseesmessage +\def\author{\global\advance\entriesinthiscollab by 1\relax% +\global\advance\allentries by 1\relax\futurelet\next\lookforbracket} + +\def\new@author@def#1#2{% + \move@AU\move@AF\move@AUAF + \let\@AF@join\@author@join + \def\@author{{\href{http://orcid.org/#1}{#2% +\openin1 Orcid-ID.png \ifeof1 +%% message for authors?? +%\typeout{^^J^^J ! Missing File: Orcid-ID.png; needed for Orcid Author icon ! +%^^J} +\else% +\hskip2pt\includegraphics[width=9pt]{Orcid-ID.png}\fi}}{}}% +}% + +\def\orciderrormessage{% +\typeout{^^J^^J [\firstarg]\space Invalid ORCID Identifier!^^J^^J The ID +should consist of four sets of four digits,^^J separated with -, ie, +0000-0012-3245-1234 or ^^J +0000-0012-3245-123X +^^J^^J +Please fix, or don't use square bracket argument with +\string\author[]\string{\string} +^^J^^J}% +} + +%% Tests to see if author gave reasonable Orcid number; +%% if not, stops processing and gives error message. +\newif\ifbadOrcid +\def\lookatOrcid #1-#2-#3-#4-{% +\def\one{#1}\def\two{#2}\def\three{#3}\def\four{#4}% +\ifx\one\empty% +\global\badOrcidtrue% +\else% +\ifx\two\empty% +\global\badOrcidtrue% +\else% +\ifx\three\empty% +\global\badOrcidtrue% +\else% +\ifx\four\empty% +\global\badOrcidtrue% +\fi\fi\fi\fi} + +\def\lookforDigits #1#2#3#4{ +\def\xone{#1}\def\xtwo{#2}\def\xthree{#3}\def\xfour{#4} +%% +\ifx\xone\empty +\global\badOrcidtrue +\else + \ifcat \xone 1\else + \global\badOrcidtrue\fi +\fi +%%% +\ifx\xtwo\empty +\global\badOrcidtrue +\else + \ifcat \xtwo 1\else + \global\badOrcidtrue\fi +\fi +%%% +\ifx\xthree\empty +\global\badOrcidtrue +\else + \ifcat \xthree 1\else + \global\badOrcidtrue\fi +\fi +%%% +\ifx\xfour\empty +\global\badOrcidtrue +\else + \ifcat \xfour 1\else + \global\badOrcidtrue\fi +\fi} + +\def\FinallookforDigits #1#2#3#4{ +\def\xone{#1}\def\xtwo{#2}\def\xthree{#3}\def\xfour{#4} +%% +\ifx\xone\empty +\global\badOrcidtrue +\else + \ifcat \xone 1\else + \global\badOrcidtrue\fi +\fi +%%% +\ifx\xtwo\empty +\global\badOrcidtrue +\else + \ifcat \xtwo 1\else + \global\badOrcidtrue\fi +\fi +%%% +\ifx\xthree\empty +\global\badOrcidtrue +\else + \ifcat \xthree 1\else + \global\badOrcidtrue\fi +\fi +%%% +\ifx\xfour\empty +\global\badOrcidtrue +\else + \ifcat \xfour 1\else + \if\xfour X + \else + \global\badOrcidtrue\fi% + \fi% +\fi} + + + + + +%% Last digit might be X +\def\xauthor[#1]#2{\def\testone{#1-}\def\firstarg{#1}% +\setbox0=\hbox{\expandafter\lookatOrcid\testone {}-{}-{}-{}- +\expandafter\lookforDigits\one {}{}{}{}% +\expandafter\lookforDigits\two {}{}{}{}% +\expandafter\lookforDigits\three {}{}{}{}% +\expandafter\FinallookforDigits\four {}{}{}{}}% +%% +\ifbadOrcid\let\go\orciderrormessage +\else\let\go\relax\fi\go% +\ifbadOrcid\let\go\stop\else\let\go\relax\fi\go% +\new@author@def{#1}{#2}}%% oct 7, this doesn't seem to work + +\def\yauthor{\@author@def{}} + +\def\altaffilmark#1{\typeout{^^J^^J\string\altaffilmark\space is no longer +needed. It will not do anything.^^J Please use +\string\altaffiliation\string{\string} instead.^^J^^J}\stop} + +\def\altaffiltext#1{\typeout{^^J^^J\string\altaffiltext\space is no longer +needed. It will not do anything.^^J Please use +\string\altaffiliation\string{\string} instead.^^J^^J}\stop} + +%% We do not need \and in list of authors. It is taken care of +%% automatically. Below is the definition from revtex4-1: +% +%\renewcommand\frontmatter@and{\class@err{\protect\and\space is not +% supported}} + +\newcount\AuthorCollaborationLimit +\let\AuthorCallLimit\AuthorCollaborationLimit +%% no limit for default +\AuthorCollaborationLimit=10000 +\newcount\largestAffilNum + +\def\lookfornumbers#1#2#3#4#5#6#7#8#9{\def\one{#1} +\def\two{#2} +\def\three{#3} +\def\four{#4} +\def\five{#5} +\def\six{#6} +\def\seven{#7} +\def\eight{#8} +\def\nine{#9} +\ifnum\one>\largestAffilNum +\global\largestAffilNum=\one\fi +%%% +\ifx\two\empty\else +\ifnum\two>\largestAffilNum +\global\largestAffilNum=\two\fi\fi +%%% +\ifx\three\empty\else +\ifnum\three>\largestAffilNum +\global\largestAffilNum=\three\fi\fi +%%% +\ifx\four\empty\else +\ifnum\four>\largestAffilNum +\global\largestAffilNum=\four\fi\fi +%%% +\ifx\five\empty\else +\ifnum\five>\largestAffilNum +\global\largestAffilNum=\five\fi\fi +%%% +\ifx\six\empty\else +\ifnum\six>\largestAffilNum +\global\largestAffilNum=\six\fi\fi +%%% +\ifx\seven\empty\else +\ifnum\seven>\largestAffilNum +\global\largestAffilNum=\seven\fi\fi +%%% +\ifx\eight\empty\else +\ifnum\eight>\largestAffilNum +\global\largestAffilNum=\eight\fi\fi +%%% +\ifx\nine\empty\else +\ifnum\nine>\largestAffilNum +\global\largestAffilNum=\nine\fi\fi +} + +%\gdef\newcomma@space{\hskip-3pt\textsuperscript{,}}% +\def\doEtAl{\rm et al.\gdef\doEtAl{\relax}} +%% ===================== +\newif\iffirsttime +\firsttimetrue +\newcount\totalentries +\newcount\docollabnum +\newcount\tempauthornumber +\newcount\countauthors +\newif\ifdothis +\def\doAnd{} +\newcount\testnum + +\def\olddoauthor#1#2#3{% +\iflongauthor\vskip6pt\fi +\global\advance\countauthors by 1 +\ifnum\countauthors>\AuthorCollaborationLimit +\doEtAl +\else +\ifnum\AuthorCollaborationLimit=1 +\let\@listand\relax +\fi + \ignorespaces\leavevmode\hbox{#1\unskip\@listcomma}% nice, keeps name from breaking across lines +\fi + \begingroup +\ifnum\countauthors>\AuthorCollaborationLimit\else + #3% all affil numbers +\ifx\@affilID@temp\empty +\else% +\setbox0=\hbox{\expandafter\lookfornumbers\@affilID@temp{}{}{}{}{}{}{}{}{}}% +\fi\fi +%% #2= \altaffiliation{} or \email{} or +%% possibly anything other than author, affiliation, or collaboration + \@if@empty{#2}{\endgroup{}{}} +{\ifnum\countauthors>\AuthorCollaborationLimit\endgroup{}{}%% <<< bug fix, added \endgroup{}{} +\else +\endgroup{\comma@space}{}\frontmatter@footnote{#2}\fi}% +\ifnum\countauthors>\AuthorCollaborationLimit\else \space +\@listand\fi +}% + +\newif\ifaddspace +\def\doauthor#1#2#3{% +\iflongauthor\vskip6pt\fi%%% +\ifanonymous% + \iffirsttime% + \global\firsttimefalse% + Anonymous author(s)% + \fi% +\else%% ends at end of this def +%%% +\ifnum\docollabnum< 1 +\global\AuthorCollaborationLimit\expandafter\csname +currCollabLimit0\endcsname% +%% this won't change until after collaboration name at end +\fi %% end ifnum\docollabnum +%% +%%%%%%%%%%%%%%%% +\global\advance\totalentries by 1\relax% +\global\advance\countauthors by 1\relax% +%%% +\ifallauthors\global\AuthorCollaborationLimit=9999 \fi% +%%% +% for testing +% [author number=\the\countauthors/ auth collab limit +% =\the\AuthorCollaborationLimit] +% +\gdef\xone{#1}% +\ifnum\countauthors < \AuthorCollaborationLimit +\global\addspacetrue +\gdef\docomma{,}\else\gdef\docomma{}\fi% ok +%%% +\ifnum\countauthors = \AuthorCollaborationLimit +\ifnum\AuthorCollaborationLimit=1\else +\gdef\doAnd{And }\fi% +\ifnum\tempauthornumber= 1 +\gdef\doAnd{ } \fi\fi% +%% +{\tempauthorminusone=\AuthorCollaborationLimit +\advance\tempauthorminusone by -1 +\ifnum\countauthors=\tempauthorminusone +\gdef\doAnd{And }% +\gdef\docomma{}\fi}% +%%% +\global\dothisfalse% +%% if num countauthors is less than or equal to \AuthorCollaborationLimit, print name +\ifnum\countauthors< \AuthorCollaborationLimit +%%% +\ifx\xone\empty\else% +\global\dothistrue% +%\expandafter\gdef\csname +%dothisaffil-\the\countauthors\the\docollab\endcsname{dothisone} + \ignorespaces\leavevmode\hbox{#1\unskip\docomma}% nice, keeps name from breaking across lines +\fi% +\fi% +%% +\ifnum\countauthors= \AuthorCollaborationLimit +%%% +\ifx\xone\empty\else +\global\dothistrue + \ignorespaces\leavevmode\hbox{\doAnd #1\unskip\docomma}%nice, keeps name from breaking across lines +\fi% +\fi% +%% ++++ +%% +\ifsuppressAffiliations\else% +\ifx\xone\empty\else% +\begingroup% +\ifnum\countauthors>\AuthorCollaborationLimit\else + #3% all affil numbers +\ifx\@affilID@temp\empty %% number following author +\else% +\setbox0=\hbox{\expandafter\lookfornumbers\@affilID@temp{}{}{}{}{}{}{}{}{}}% +\fi\fi% +%% #2= \altaffiliation{} or \email{} or +%% possibly anything other than author, affiliation, or collaboration + \@if@empty{#2}{\endgroup{}{}}% +{\ifnum\countauthors>\AuthorCollaborationLimit\endgroup{}{}%% <<< bug fix, added \endgroup{}{} +\else +\endgroup{\comma@space}{}\frontmatter@footnote{#2}\fi}% +\fi%% end test of empty +\fi%% end test of suppressAffiliations +%%%%%%%%%%%%%%%%%%%%%%%% +%%% Collaboration name is always used if available: +\expandafter\ifx\csname currCollabName\the\totalentries\endcsname\relax\else +%%% +%%% +%%% +%% changed locally: +{\advance\docollabnum 1 +\advance\countauthors-1 +%%% +%%% We need to test to see if more than one author in collaboration +%%% and if the number of authors is greater than the \AuthorCollaborationLimit. +%%% If both of these are true, than use `et al.' , otherwise do not: +\expandafter\ifx\csname +CollabTotalAuthors\the\docollabnum\endcsname\relax +\else +\expandafter\ifnum\csname +CollabTotalAuthors\the\docollabnum\endcsname +< 2 %%%%% Don't use et al if there is only one author +\else +\expandafter\ifnum\csname CollabTotalAuthors\the\docollabnum\endcsname +>\AuthorCollaborationLimit\relax% +\ifnum\AuthorCollaborationLimit=0\else +\vskip3pt +{\rm et al.} \vskip-3pt +\fi\fi\fi\fi% +}%% end local change to docollabnum +%%%% +\expandafter\ifx\csname +currCollabName\the\totalentries\endcsname\empty +\vskip-3pt +\else +\vskip6pt +\expandafter\csname currCollabName\the\totalentries\endcsname\vskip8pt +\affiliation{testing} +\fi% +%%%%%%%% +\global\countauthors=0 +%%% +%%% +\global\advance\docollabnum by 1 +%% Set up counters for next time through this loop: +{\advance\docollabnum by1 + \expandafter\ifx\csname + specificCollabLimit\the\docollabnum\endcsname\relax + \else + \global\AuthorCollaborationLimit=\csname + specificCollabLimit\the\docollabnum\endcsname + \fi% +\expandafter\ifx\csname +CollabTotalAuthors\the\docollabnum\endcsname\relax +\else +\global\tempauthornumber=\csname +CollabTotalAuthors\the\docollabnum\endcsname +\fi}% +\fi %% ends test to see if it is time to use collaboration name +\fi %% ends ifanonymous +\ifaddspace\ \fi\global\addspacefalse}% oct 7, 2020, allows multiple names to break over lines, + %but no extra space if \collaboration{1} + + +%%%% ++++==== +\newcount\tempauthorminusone +%% +++ +\def\doAllauthors#1#2#3{% +\global\suppressAffiliationsfalse +\iflongauthor\vskip6pt\fi +%%% +\ifanonymous + \iffirsttime + \global\firsttimefalse + Anonymous author(s) + \fi +\else %% ends at end of this def +%%% +\ifnum\docollabnum< 1 +%% these won't change until after collaboration name at end +\global\AuthorCollaborationLimit\expandafter\csname currCollabLimit0\endcsname +\global\tempauthornumber=\csname CollabTotalAuthors1\endcsname +\fi%% end ifnum\docollabnum +%% +%%%%%%%%%%%%%%%% +\global\advance\totalentries by 1 +\global\advance\countauthors by 1 +%%% +\ifallauthors\global\AuthorCollaborationLimit=9999 \fi +%%% +% for testing +%[author number=\the\countauthors/ temp author +%=\the\tempauthornumber] +\def\one{#1} +{\tempauthorminusone=\tempauthornumber +\advance\tempauthorminusone by -1 +\ifnum\countauthors < \tempauthornumber +\gdef\xdocomma{,}% +\else\gdef\xdocomma{}\fi% +%%% +\ifnum\countauthors = \tempauthornumber +\gdef\xdoAnd{And}\gdef\xdocomma{}% +\else\gdef\xdoAnd{}\fi% +\ifnum\tempauthornumber= 1 +\gdef\xdoAnd{}\gdef\xdocomma{}\fi% +\ifnum\countauthors=\tempauthorminusone +\gdef\xdocomma{}\fi% +} +%%% +%% if num countauthors is less than or equal to \AuthorCollaborationLimit, print name +\ifnum\countauthors< \AuthorCollaborationLimit +%%% +\ifx\one\empty\else + \ignorespaces\leavevmode\hbox{\unskip\xdoAnd\ #1\unskip\xdocomma}% nice, keeps name from breaking across lines +\fi\fi% +%% +\ifnum\countauthors= \AuthorCollaborationLimit +%%% +\ifx\one\empty\else +\ignorespaces\leavevmode\hbox{\unskip\xdoAnd\ #1\unskip\xdocomma}% nice, keeps name from breaking across lines +\fi% +\fi% +%% +\ifx\one\empty\else + \begingroup +\ifnum\countauthors>\AuthorCollaborationLimit\else + #3% all affil numbers +\ifx\@affilID@temp\empty +\else% +\setbox0=\hbox{\expandafter\lookfornumbers\@affilID@temp{}{}{}{}{}{}{}{}{}}% +\fi\fi +%% #2= \altaffiliation{} or \email{} or +%% possibly anything other than author, affiliation, or collaboration + \@if@empty{#2}{\endgroup{}{}} +{\ifnum\countauthors>\AuthorCollaborationLimit\endgroup{}{}%% <<< bug fix, added \endgroup{}{} +\else +\endgroup{\comma@space}{}\frontmatter@footnote{#2}\fi}% +\fi%% end test of empty +%%%%%%%%%%%%%%%%%%%%%%%% +%%% Collaboration name is always used if available: +\expandafter\ifx\csname currCollabName\the\totalentries\endcsname\relax\else +%%% +%% No et al in allauthors, because all authors are listed! +%% +\expandafter\ifx\csname +currCollabName\the\totalentries\endcsname\empty +\else +\vskip6pt +\expandafter\csname currCollabName\the\totalentries\endcsname\vskip6pt +\fi +\global\countauthors=0 +%%% +%%% +\global\advance\docollabnum by 1 +%% Set up counters for next time through this loop: +{\advance\docollabnum by1 + \expandafter\ifx\csname + specificCollabLimit\the\docollabnum\endcsname\relax + \else + \global\AuthorCollaborationLimit=\csname + specificCollabLimit\the\docollabnum\endcsname + \fi +% +\expandafter\ifx\csname +CollabTotalAuthors\the\docollabnum\endcsname\relax +\else +\global\tempauthornumber=\csname +CollabTotalAuthors\the\docollabnum\endcsname +\fi} +\fi %% ends test to see if it is time to use collaboration name +\fi %% ends ifanonymous +}% + +%%% +%% set \affil to match \affiliation found in revtex, since authors are accustomed to using \affil{} +\let\affil\affiliation + +\newif\iffirstaffil +\firstaffiltrue + +\newcount\affilnum +%% +++! +\def\@affil@script#1#2#3#4{% +\ifsuppressAffiliations\else +\iffirstaffil +% Oct 2017 +\vskip2pt +\global\firstaffilfalse\fi + \@ifnum{#1=\z@}{}{% + \par + \begingroup + \frontmatter@affiliationfont + \@ifnum{\c@affil<\affil@cutoff}{}{% +\def\one{#1} +%% +%% +\ifnum\one<\largestAffilNum +%% this makes the numbers + \def\@thefnmark{#1}\@makefnmark\fi +\ifnum\one=\largestAffilNum + \def\@thefnmark{#1}\@makefnmark\fi + }% +\ifnum\one<\largestAffilNum + \ignorespaces#3% +\fi +\ifnum\one=\largestAffilNum + \ignorespaces#3% +\fi + \@if@empty{#4}{}{\frontmatter@footnote{#4}}% + \par + \endgroup + }% +\fi}% + + + +\newif\ifnobreakafterkeywords +\def\NoNewPageAfterKeywords{\global\nobreakafterkeywordstrue} +\NoNewPageAfterKeywords +\def\NewPageAfterKeywords{\global\nobreakafterkeywordsfalse} + +%%%+++!!! +\def\frontmatter@maketitle{% +%% \@author@finish needs to be here: +\@author@finish +\if@firstsection% not appendix, in other words + \title@column\titleblock@produce +\onecolumngrid +\else +% +\global\firstaffiltrue + \title@column\secondtitleblock@produce +\fi + \suppressfloats[t]% +%% Prevent these from being turned off so that +%% we can use \maketitle again for \AllAuthors. +%% +% \let\and\relax + \let\affiliation\@gobble + \let\author\@gobble +% \let\@AAC@list\@empty +% \let\@AFF@list\@empty +% \let\@AFG@list\@empty +% \let\@AF@join\@AF@join@error +% \let\email\@gobble +% \let\@address\@empty +% \let\maketitle\relax +% \let\thanks\@gobble +\if@firstsection +\let\abstract\@undefined\let\endabstract\@undefined +\titlepage@sw{% +\ifnobreakafterkeywords +\else +\vfil +\ifrnaas\else \clearpage\fi +\fi + }{}% +\fi +}% + + +\let\maketitle\frontmatter@maketitle + +\def\secondtitleblock@produce{% + \begingroup + \ltx@footnote@pop + \def\@mpfn{footnote}% + \def\thempfn{\thefootnote}% + \c@footnote\z@ + \let\@makefnmark\frontmatter@makefnmark +% \frontmatter@setup + \thispagestyle{titlepage}%\label{FirstPage}% +% \frontmatter@title@produce + \groupauthors@sw{% + \frontmatter@author@produce@group + }{% + \frontmatter@author@produce@script + }% + \endgroup +}% + +%% no club or widow lines +\widowpenalty=10000 +\clubpenalty\widowpenalty +\setlength{\footnotesep}{8pt} + +\ifmodern +\setlength{\voffset}{0in} +\setlength{\hoffset}{0in} +\setlength{\textwidth}{6in} +\setlength{\textheight}{9.2in} +\setlength{\headheight}{0ex} +\setlength{\headsep}{36pt} % this is 2 lines in ``manuscript'' +\setlength{\footnotesep}{0in} +\setlength{\topmargin}{-\headsep} +\setlength{\oddsidemargin}{0.25in} +\setlength{\evensidemargin}{0.25in} +\setlength{\parindent}{0.54\baselineskip} +\sloppy\sloppypar +\fi + + +\def\figurename{Figure} +\def\tablename{Table} +\def\fnum@figure{{\bf\figurename~\thefigure}} +\def\fnum@table{{\bf\tablename~\ifappletter\thesection\fi\thetable}} + + +\def\tempfootmark#1{} + +\newcount\c@affilcount +\renewcommand*\altaffiliation[2][]{% +\@AF@join{\ifanonymous\else +#1#2\ifmodern\baselineskip=14pt\fi +\if@two@col\hsize=.5\textwidth +\advance\hsize by -18pt +\fi\fi}% +}% + + +\def\correspondingauthor#1{{\ifanonymous +\else +\renewcommand\thefootnote{\hskip-12pt} +\footnote{Corresponding author: #1\ifmodern\vrule depth 5pt +width 0pt\relax\fi}\fi}} + +\let\saveemail\email +\def\email#1{\ifanonymous +\else{\let\ltx@footmark\tempfootmark +\saveemail{}} +{\renewcommand\thefootnote{\hskip-12.1pt} +\footnote{\href{mailto: #1}{#1}\ifmodern\vrule depth 7pt width +0pt\relax\else\ifmanu\vskip-4pt\else\vrule depth 7pt width +0pt\fi\fi}}\fi} + +\def\nocollaboration#1{% +\collaboration{#1}{\vbox to +0pt{\vss\centerline{---}\vskip2pt}} +} + +%% May 19 +%% \AuthorsAndCollaboration changed to \FullCollaborationID +%% June 6 \FullCollaborationID changed to \xcollaboration{}{} +%% june 7 \collaboration changed to \xcollaboration; fullcollaborationid changed to \collaboration + +%% here just in case we need it in the future... +\def\xcollaboration#1#2{ +\global\advance\allentries by 1 +\expandafter\def\csname +currCollabLimit\the\allentries\endcsname{#1} +\@author@def{\@booleantrue +\collaboration@sw}{#2} +} + +\let\savelistand\@listand +\newcount\numauthors +\newcount\collabnum +\newbox\collabnamebox +\newif\iffirstcollab +\global\firstcollabtrue + +\newif\ifcollaborationon +\def\collaboration#1#2{\global\collaborationontrue +\global\advance\collabnum by 1 +\iffirstcollab\global\firstcollabfalse +\expandafter\xdef\csname currCollabLimit0\endcsname{#1} +\fi +%% make this def so that we can use it when we want in doauthor: +\expandafter\gdef\csname specificCollabLimit\the\collabnum\endcsname{#1} +%% This allows us access the number of authors per collaboration: +\expandafter\xdef\csname +CollabTotalAuthors\the\collabnum\endcsname{\the\entriesinthiscollab} +\global\entriesinthiscollab=0 +%% +\global\advance\allentries by 1 +%% +%% we should have only one of these with this number; this used to say when +%% use specificCollabLimit: +\expandafter\gdef\csname currCollabLimit\the\allentries\endcsname{#1} +%% we should have only one of these with this number +\expandafter\gdef\csname +currCollabName\the\allentries\endcsname{%\ifnum#1>0 +%\sc And the\vskip4pt\fi +#2} +%% +\let\doEtAl\relax +%% not here +\@author@def{\@booleanfalse +\collaboration@sw}{}} + + +\def\and{ +\centerline{\vbox {\vrule height 12pt width0pt and\vskip2pt}} +} + +%\def\andthe{% +%\collaboration{\vbox {\vrule height 12pt width0pt and +%the\vskip2pt}}\vskip4pt +%} + +%% gets rid of () around collaboration +\def\@collaboration@present#1#2#3#4{% +\par + \begingroup +\vskip3pt +\iflongauthor\vskip-4pt\ifmodern\vskip-6pt\fi\fi + \frontmatter@collaboration@above + \@affilID@def{}% + \@tempcnta\z@ + \@author@present{}{\ignorespaces#3\unskip}{#4}% +%% October 2017 + \par +\ifmodern%\vskip-4pt +\else +\iflongauthor\else\vskip-6pt\fi\fi + \endgroup +\iflongauthor +\else\vskip8pt\fi + \set@listcomma@list#1% +\vskip1pt %% was \vskip9pt +}% + + +%%% These lines were commented out until a fix could be applied that +%%% addresses the underlying issues. The problem is that on Linux systems +%%% you can not write a "hidden" .bib file. There is no issue with this +%%% on Mac OS X nor Windows. +%%% get rid of \jobname Notes being sent to .aux file: +%\let\bibdata@app\relax +%\def\pre@bibdata{} + +%% This is the underlying issue: +%% Redefining \@bibdataout@init will keep useless file, \jobnameNotes, from being written. +\let\@bibdataout@init\relax + +%% redefining and simplifying RevTeX4-1 definition, so that bibliography is not looking for +%% \jobnameNotes: + +\def\bibliography#1{\bibliography@latex{#1}}% + + +%%% +\newif\iffrontmatterfirsttime +\global\frontmatterfirsttimetrue +\let\savecentercr\@centercr +\def\frontmatter@author@produce@script{% + \begingroup + \let\@author@present\@author@present@script + \frontmatterverbose@sw{\typeout{\string\frontmatter@author@produce@script:}\say\@AAC@list\say\@AFF@list\say\@AFG@list}{}% + \let\AU@temp\@empty + \@tempcnta\z@ + \let\AF@opr \@gobble + \def\AU@opr{\@author@count\@tempcnta}% + \def\CO@opr{\@collaboration@count\AU@temp\@tempcnta}% + \@AAC@list + \expandafter\CO@opr\@author@cleared + \begingroup + \frontmatter@authorformat + \let\AF@opr \@affilID@def + \let\AU@opr \@author@present + \def\CO@opr{\@collaboration@present\AU@temp}% + \set@listcomma@list\AU@temp + \@AAC@list +%% \, added to definition taken from revtex4-1 to prevent error message. +\, \unskip\unskip + \par + \endgroup +%% below + \begingroup + \frontmatter@above@affiliation@script + \let\AFF@opr \@affil@script +{\parskip=2pt +\def\@centercr{\vrule depth 3pt width0pt\vskip1sp} + \@AFF@list} +\let\@centercr\savecentercr +%% sept 14, 2020 +\iffrontmatterfirsttime +\frontmatter@footnote@produce +\global\frontmatterfirsttimefalse +\fi + \par + \endgroup + \endgroup +}% + +\let\auto@bib\relax + +\newif\iffirstaffil +\firstaffiltrue +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% + +%% These commands were in aastex earlier; I redefined. +\def\tighten{\global\tightentrue\normalsize} +\let\tightenlines=\tighten +\def\singlespace{\par\global\doublespacefalse\global\tightenfalse\normalsize} +\def\doublespace{\par\global\doublespacetrue\global\tightenfalse\normalsize} + +\bibliographystyle{aasjournal} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%% October 2017 + +\renewenvironment{widetext}{% +\if@two@col + \par\ignorespaces + \setbox\widetext@top\vbox{% + \hb@xt@\hsize{% + \leaders\hrule\hfil + \vrule\@height6\p@ + }% + }% + \setbox\widetext@bot\hb@xt@\hsize{% + \vrule\@depth6\p@ + \leaders\hrule\hfil + }% + \onecolumngrid + \vskip10\p@ + \dimen@\ht\widetext@top\advance\dimen@\dp\widetext@top + \cleaders\box\widetext@top\vskip\dimen@ + \vskip6\p@ + \prep@math@patch +\fi}{% +\if@two@col + \par + \vskip6\p@ + \setbox\widetext@bot\vbox{% + \hb@xt@\hsize{\hfil\box\widetext@bot}% + }% + \dimen@\ht\widetext@bot\advance\dimen@\dp\widetext@bot + \cleaders\box\widetext@bot\vskip\dimen@ + \vskip8.5\p@ + \twocolumngrid\global\@ignoretrue + \@endpetrue +\fi}% +\newbox\widetext@top +\newbox\widetext@bot + +\urlstyle{rm} + +\def\doi#1{\href{https://doi.org/#1}{https://doi.org/#1}} +\let\savedoi\doi + +\def\mdash{---} + +\newif\ifcenterwidetable +%% these two definitions are the same, but it might +%% be convenient to have both +\def\centerwidetable{\global\centerwidetabletrue} + + +%% this doesn't seem to be documented, assume we don't need it: +%\def\centernarrowtable{\global\centerwidetablefalse} + +%% default, center within width of text on both sides + \def\LT@LR@c{\LTleft=0pt plus1fill + \LTright\LTleft}% + +\def\widetable{\def\LT@LR@c{\LTleft=0pt minus1fill + \let\LTright\LTleft}} + +\newif\ifreturntotwocol + + +%%%%%%%%% +%% to help with graceful linebreaks in two column text: + \tolerance 9999% +%% sloppy defines emergencystretch to be 3 em, this is a bit +%% more conservative: + \emergencystretch 1em + \hfuzz .5\p@ + +%%%%%%%%% +%% Nominal Conversion Constants + +%% \boldmath inside the \hbox ?? +\def\nomSolarEffTemp{\leavevmode\hbox{\boldmath$\mathcal{T}^{\rm N}_{\mathrm{eff}\odot}$}} +\def\nomTerrEqRadius{\leavevmode\hbox{\boldmath$\mathcal{R}^{\rm N}_{E\mathrm e}$}} +\def\nomTerrPolarRadius{\leavevmode\hbox{\boldmath$\mathcal{R}^{\rm N}_{E\mathrm p}$}} +\def\nomJovianEqRadius{\leavevmode\hbox{\boldmath$\mathcal{R}^{\rm +N}_{J\mathrm e}$}} + \def\nomJovianPolarRadius{\leavevmode\hbox{\boldmath$\mathcal{R}^{\rm + N}_{J\mathrm p}$}} + \def\nomTerrMass{\leavevmode\hbox{\boldmath$(\mathcal{GM})^{\rm N}_{\mathrm E}$}} + \def\nomJovianMass{\leavevmode\hbox{\boldmath$(\mathcal{GM})^{\rm N}_{\mathrm J}$}} + \def\Qnom{\leavevmode\hbox{\boldmath$\mathcal{Q}^{\rm N}_{\odot}$}} +\let\Qn\Qnom + +%% Generic commands that can be given an argument: +\def\nom#1{\leavevmode\hbox{\boldmath$\mathcal{#1}^{\rm N}_{\odot}$}} +\def\Eenom#1{\leavevmode\hbox{\boldmath$\mathcal{#1}^{\rm N}_{Ee}$}} +\def\Epnom#1{\leavevmode\hbox{\boldmath$\mathcal{#1}^{\rm N}_{Ep}$}} +\def\Jenom#1{\leavevmode\hbox{\boldmath$\mathcal{#1}^{\rm N}_{Je}$}} +\def\Jpnom#1{\leavevmode\hbox{\boldmath$\mathcal{#1}^{\rm N}_{Jp}$}} + +%%%%%%%%%%%%%%%% +%% Ability to have tables, equations, figures in appendix start from 1, and use appendix section letter. + +\newif\ifappletter +\def\apptablenumbers{\global\applettertrue +\setcounter{table}{0} +\setcounter{figure}{0} +\setcounter{equation}{0} +\def\thetable{\thesection\the\c@table}% +\def\fnum@table{{\bf\tablename~\thetable}}% +\def\thefigure{\thesection\the\c@figure}% +\def\fnum@figure{{\bf\figurename~\thefigure}}% +}% + +%%% easier to remember than \apptablenumbers +\let\restartappendixnumbering\apptablenumbers + +\def\resetapptablenumbers{\global\c@table=0 +\global\c@figure=0 +\global\c@equation=0 +\def\thetable{\thesection\the\c@table} +\def\fnum@table{{\bf\tablename~\thetable}}% +\def\thefigure{\thesection\the\c@figure} +\def\fnum@figure{{\bf\figurename~\thefigure}}% +} + +%% written for aastex63 +\newif\ifallauthors +\def\allauthors{ +\global\allauthorstrue +\let\doauthor\doAllauthors +\ifanonymous +\vskip6pt\vskip1sp\centerline{\large\bf All Authors and +Affiliations\vrule depth 18pt width0pt}\nobreak +\centerline{Anonymous author(s)} +\else +\ifnumlines\nolinenumbers\fi +\onecolumngrid +\clearpage +{\vskip6pt\vskip1sp\centerline{\large\bf All Authors and +Affiliations\vrule depth 18pt width0pt}\nobreak +\global\docollabnum=0 +\global\totalentries=0 +\global\countauthors=0 +\maketitle +}\fi} + +%% written for AASTeX62 +\def\oldallauthors{%% this conditional keeps \allauthors from turning on +%% unless \AuthorCollaborationLimit is used: +\ifnumlines\nolinenumbers\fi +\onecolumngrid +\clearpage +\AuthorCollaborationLimit=10000 +%\largestAffilNum=10000 <<== not needed +{\vskip6pt\vskip1sp\centerline{\large\bf All Authors and +Affiliations\vrule depth 18pt width0pt}\nobreak +\maketitle +}} +\let\AllAuthors\allauthors + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% Highlight Figure +\definecolor{ltblue}{cmyk}{.5,.1,.1,0} +\newdimen\currwidth +\long\def\highlightfigure#1{ +\bgroup +\fboxrule=4pt +\fboxsep=12pt +\vskip6pt +\global\currwidth=\hsize +\global\advance\currwidth by -32pt +\noindent\hbox to\currwidth{\fcolorbox{ltblue}{white}{% +$\vcenter{\hbox to\currwidth{\hss#1\hss}}$}} +\egroup} + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% New interactive command: + +\def\xlc{lc} +\def\xjs{js} +\def\xanimation{animation} +\newbox\interactbox +\newif\ifcorrectentries + + +\def\interactive#1#2{ +\global\correctentriesfalse\def\checkone{#1} +\ifx\checkone\xlc\correctentriestrue\fi +\ifx\checkone\xjs\correctentriestrue\fi +\ifx\checkone\xanimation \correctentriestrue\fi +\def\checktwo{#2} +\ifx\checktwo\empty\global\correctentriesfalse\fi +\ifcorrectentries +\else\hrule height1pt\vskip12pt\bf ERROR: +The command +{\tt\string\begin\string{interactive\string}\string{\string}\string{\string}} +needs two arguments. The +first describes the interactive type and the only allowed choices are +lc, js, or animation.\\ +The second argument is the movie file or package +containing the interactive figure components. See\\ +\url{https://journals.aas.org/aastexguide/\hashmark interactivefig} for more +details. +\vskip12pt\hrule height1pt +\fi \global\currwidth\hsize +\global\advance\currwidth by -32pt +%% we need to set \currwidth here because interactbox expands +%% before highlightfigure +\global\setbox\interactbox=\vbox\bgroup\hsize=\currwidth\relax\centering +} + +\def\endinteractive{\egroup +\ifcorrectentries\highlightfigure{\copy\interactbox}\fi +} + +%%%% For cases in which footnotes are called in full width environment +%% but are used in two cols. This keeps them from overwriting the +%% second column: + +\let\savefootnote\footnote +\def\onecolfootnote#1{\savefootnote{\hsize=.5\textwidth\advance\hsize +by-18pt\relax#1}} + +\def\onecolumnfootnotes{\let\footnote\onecolfootnote} + +\newdimen\movetableright + +%% for anonymous option +\newif\ifsuppressAffiliations +\def\suppressAffiliations{\global\suppressAffiliationstrue} + +%% new definition to be used in trackchanges: +\def\sout#1{\raise5pt\hbox{\underline{\vbox to +0pt{\vskip-4pt\hbox{#1\vrule height 8.5pt depth 3.5pt width0pt}\vss}}}} + +%% changes for affiliations when anonymous option is used: +\ifanonymous +\suppressAffiliationstrue +\gdef\affiliation#1{}%% may 20, 2020 +\def\xauthor[#1]#2{} +\let\yauthor\@gobble +\def\lookforbracket{\ifx\next[ +\let\go\xauthor\else\let\go\yauthor\fi\go} +\def\author{\futurelet\next\lookforbracket} +\fi + + +%%%%%%%%%%%%% +%% Line numbering + + +\ifnumlines +\usepackage[mathlines]{lineno}%% dec 20 +%% +\linenumbers*[1] +%%\linenumbersep default=10pt +\if@two@col +\advance\linenumbersep -6pt +\else +\advance\linenumbersep 12pt +\fi +\fi + +%% Use when line numbers are on, and after \usepackage{amsmath}. +%% Will make line numbering work on math as it would without amsmath. +\def\fixmathlinenumbering{ +\let\saveopensqbracket\[ +\def\[{\linenomath\saveopensqbracket} +\let\saveequation\equation +\let\saveendequation\endequation +%% + \let\savealign\align + \let\saveendalign\endalign +%% + \let\savealigned\aligned + \let\saveendaligned\endaligned +%% +\def\align{\linenomath\savealign} + \def\endalign{\saveendalign} + \def\aligned{\linenomath\savealigned} + \def\endaligned{\linenomath\saveendaligned} +%% +\def\equation{\linenomath\saveequation} +\def\endequation{\linenomath\saveendequation} +\usepackage[mathlines]{lineno} +} + +\AtBeginDocument{\expandafter\ifx\csname +@amsmath@err\endcsname\relax\else\fixmathlinenumbering\fi} + +\endinput +%% Change Log +============================ +Jan 29, 2021 +added \ifonecolstyle to see if reference numberlines need to +be closer to text + +Dec 20, 2020 +Line numbering solutions: + +Line numbering equations and \[ \] works fine. + +$$math $$ does not work, and should be replaced with \[ math \] + +If author has \usepackage{amsmath} the equations will not number; +amsmath and lineno are incompatible. + + +June 28 +For using \edit{}{} in section heads; new command, +\simpleedit that will prevent errors in section heads +and in bookmarks. \edit is set to be equal to \simpleedit{}{} +in \section definition, so nothing needs to be done by user. +\protect used in section head, as \protect\edit{}{}, is not +necessary. + +June 27 +\null added to \end{deluxetable} and \csname enddeluxetable*\endcsname +to force final page of multipage table to print. + +June 26 +Acknowledgments: remember to use +\begin{acknowledgments}...\end{acknowledgments} form +OR +\begin{acknowledgements}...\end{acknowledgements} + +Now have an error message built in if someone uses +just \acknowledgments or \acknowledgements + + +June 4, 2020 + Added \nocollaboration{0} to first + section head, if anonymous was true. This + allowed correct titlepage for anonymous + if any style option was used. + +Acknowledgments: remember to use +\begin{acknowledgments}...\end{acknowledgments} form + + + + +%% Change Log +============================ +May 19, 2020 +Changed definition of \sout (strike out) so that +it works with a variety of citations in +argument of \deleted and \replaced without complaint. + +Made anonymous work with \longauthor, and without +\collaboration or \nocollaboration. + +Changed \acknowledgements to +\begin{acknowledgements}...\end{acknowledgements} +(More error proof, and standard mark up) + +++++++++++++++++++++++++++++++++++++++++++++++++++++++++ + +June 8, 2019 +Changed \author and \collaboration macros. +Collaboration now takes two arguments: +#1= number of authors to be listed before the +name of the collaboration; #2 = name of the collaboration + +\nocollaboration{} has one argument, +#1= the number of authors above it that we want to print on the title page. + +June 6, 2019 + +\acknowledgments does not use \begin{}...\end{} form, +now just \acknowledgments command. Acknowledgments text +ends with \par, so if author wants more than one paragraph +in acknowledgment he/she should surround text with curly +bracket: + +\acknowledgments +text... + +or + +\acknowledgments +{text... + +more text...} + +------ + + +============================ +June 3, 2019 +\let\footnote\onecolfootnote on page where references start, but +before footnotes are entered, +will allow footnotes to break in the right place (one column's width). + +============================ +May 15, 2019 +\centerwidetable is now \movetableover at Greg's suggestion. + +============================ +Nov 27, 2017 + +1) Change to \begin{widetext}...\end{widetext} to +return the horizontal lines before and after the +environment. + +2) \NoNewPageAfterKeywords is now default; +authors wanting a new page after keywords can +use the \NewPageAfterKeywords command. + +3) Change in definition names, returning to earlier version: +\turnoffediting will turn off colors for all levels +of editing mark up made with \edit1{}, \edit2{}, or \edit3{}. +You can turn off any level of editing with +\turnoffeditone, \turnoffedittwo, and \turnoffeditthree. + +4) It is now possible to use \doi{} as an argument of \dataset. +\dataset[]{\doi{10.5281/zenodo.831784}} and +\dataset[\doi{10.5281/zenodo.831784}]{\doi{10.5281/zenodo.831784}} +will work. + +============================ +October 15, 2017 + +1) \movetabledown now works with longrotatetable as it does with +rotatetable. +\movetabledown= before either +\begin{rotatetable} or +\begin{longrotatetable} + +Added \clearpage before \begin{rotatetable} and \begin{rotatetable*} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +2) + +\NoNewPageAfterKeywords, used after \documentclass{AASTeX62}, +will keep a new page from starting after keywords. +Extra vertical space before first section in Modern option. + +Solution suggested by Alex Drlica-Wagner. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +3)\edit1{}, \edit2{} and \edit3{} will add color +to the edited text. + +To get rid of the color, but not the text, authors should +use \turnoffeditonecolor (for \edit1{}) + \turnoffedittwocolor (for \edit2{}) + \turnoffeditthreecolor (for \edit3{}) +These commands have the same results as +\turnoffeditone, \turnoffedittwo, and \turnoffeditthree +which are not disabled, but the new commands make the +action to be produced more descriptive. + +Similarly, instead of \turnoffedit or \turnoffedits +we now have \turnoffeditcolors. The original two +commands still work, but the new command is more +descriptive of the results. + +Authors should be instructed to put these commands before +\begin{document} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +4) +\begin{widetext}...\end{widetext} + +\begin{widetext} +will go from twocolumngrid to onecolumngrid, centered. + +\end{widetext} will turn off centering and go back +to twocolumngrid. + +Only needed in twocolumn styles; nothing will happen +in single column styles. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +5) Sean Lake's problem with \mag was solved by Barbara Beeton online, + +``the latest edit identifies the problem unambiguously: \mag is a tex +primitive, and shouldn't be redefined. why this didn't appear in the +logs you posted is beyond me, but if you rename your command to (say) +\Mag it should stop having a problem. � barbara beeton Feb 22'' + +\mag is a tex primitive, and it is expecting to be followed by a +number. + +This had nothing to do with AASTeX61.cls + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +6) +\def\arraystretch{.9} as requested will make the space between +lines in tables shrink to 90% of the original space. + +I think what is really wanted is \def\arraystretch{1.1} which will +still give us 110% of the original space, a little extra vertical space, but not +as much as we had before. + +Meanwhile, an author can change the definition of \arraystretch{} +for a single table or all the tables in his paper, if he wants more +or less space. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +7) Abstract is now the same width as in emulateapj +in all styles, with the exception of the modern option +which is unchanged. Abstracts in all styles will break over pages +in this version. + +Thanks to suggestion by Patricio Cubillos. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +8) Center and tighten affiliations, changed and +tested for all styles, including longauthor option. + +samples.zip show examples titlepage of each style with and +without longauthor option. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +9) preprintnumbers activated. +No need to use a documentclass option. + +Just enter \reportnum{}, before \begin{document} +and repeat as many times as needed. The entries will stack +in the top right hand corner of the titlepage, for all styles. + +ie +\reportnum{YOUR-INST-REP-789} +\reportnum{MY-INST-REP-123} + +%% author can continue with as many entries as desired. +% \reportnum{A number of other numbers} +% \reportnum{More Numbers} + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +10) Title is no longer uppercase by default. It is +now title case, which means all important words are +capitalized by author. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +11) \AuthorCollaborationLimit now +set to default of 10,000. If smaller number of +authors wanted, \AuthorCollaborationLimit can +be set to the number wanted; \allauthors typed +at end of article will make every author and +affiliation print. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +12) \startlongtable\deluxetable now works in appendix, even +when it is the last entry in the paper. Added \null +to \endlongdeluxetable which has the effect of making +last page print. + +This works in my test, but it +may be useful to see the example from author, github #54 + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +13) Deluxetable no longer crashes if author has neglected +to put in \\ before \enddata. I added the non-redundant \\ +command, \crcr, and sample now works. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +14) \tablehead in deluxetable had too much space underneath +double horizontal lines. Made custom negative skip based +on each style, tested, and supplied tabsamples.zip showing +tableheads in each style. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +15) \urlstyle{rm} is set so that url and href produce +the same fonts. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +16) Fix to \dataset so that square brackets +are not printed in the case of argument +in square brackets. + +Now +\dataset[]{http://www.texnology.com} +produces +[DATASET] linked to www.texnology.com + +\dataset[TeXnology]{http://www.texnology.com} +produces +TeXnology linked to www.texnology.com + +%% This will also work, +% same results as \dataset[]{http://www.texnology.com} +% but using the more common LaTeX syntax: + +\dataset{http://www.texnology.com} +also produces +[DATASET] linked to www.texnology.com + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +17) New version of DOI: + +\doi{10.5281/zenodo.831784} +now produces hyperlinked + +https://doi.org/10.5281/zenodo.831784 + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +18) Added to definition of \software, +working with sample from August Muench, reduced +the space between words, and got rid of +extra space after punctuation with the +\frenchspacing command. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +19) August Muench entered a bug report +complaining that \clearpage doesn't always +work, but he didn't have a sample, so I am +not able to debug this one. It may be that +the problem isn't with the code, but with +the way the commands were entered, but +without a sample I have no way of knowing. + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +20) +Tested \startlongtable in all styles +and didn't find a problem with centering. +I did add a skip at the beginning of +\startlongtable in case someone didn't +leave a blank line before using the +command. + +============================ +September 21, 2016 +Finishing Version 6.1 update + +===================== +August 27, 2016 +Many changes + +===================== +August 17 +Many changes: + +%% note: +%% this keeps tables from being set to \small, code used in Revtex4-1 +\let\table@hook\relax + +===================== +Feb 29, changes to table macros to center caption even if table is wider than +width of text; give error message if user asks to rotate table but +forgets to use \floattable before table; make rotating table be full +text width even if called for in double columns. + +March 1, reworking figure and table numbering for appendices. +Deleted recent definition of \appendix, returned to earlier version +with additions. + +================ + + + + + + +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%% New interactive command: + +\def\xlc{timeseries} +\def\xjs{js} +\def\xanimation{animation} +\newbox\interactbox +\newif\ifcorrectentries + +\def\interactive#1#2{ +\global\correctentriesfalse\def\checkone{#1} +\ifx\checkone\xlc\correctentriestrue\fi +\ifx\checkone\xjs\correctentriestrue\fi +\ifx\checkone\xanimation \correctentriestrue\fi +\ifcorrectentries +\else\hrule height1pt\vskip12pt\bf ERROR: Your choices for the first argument for +{\tt\string\interactive} are timeseries, js, or animation.\\[6pt] Please choose one +of these terms.\vskip12pt \fi +%%% +\def\checktwo{#2} +\ifx\checktwo\empty \vskip12pt \bf ERROR: The command {\tt\string\interactive} needs +two arguments, with the second argument for the graphics file or files +needed.\vskip12pt\hrule height1pt \else\global\correctentriestrue\fi +\global\currwidth\hsize +\global\advance\currwidth by -32pt +%% we need to set \currwidth here because interactbox expands +%% before highlightfigure +\global\setbox\interactbox=\vbox\bgroup\hsize=\currwidth\centering} + +\def\xxinteractive#1#2{\global\correctentriesfalse\def\checkone{#1} +\ifx\checkone\xlc\correctentriestrue\fi +\ifx\checkone\xjs\correctentriestrue\fi +\ifx\checkone\xanimation \correctentriestrue\fi +\ifcorrectentries +\else\hrule height1pt\vskip12pt\bf +\noindent ERROR:\\[6pt] Your choices for the first argument for +{\tt\string\begin\string{\string\interactive\string}} are timeseries, js, or animation.\\[6pt] Please choose one +of these terms.\vskip12pt \fi +%%% +\def\checktwo{#2} +\ifx\checktwo\empty \vskip12pt \bf +\noindent ERROR:\\[6pt] +The second argument of %{\tt\string\begin\string{interactive\string}} is the file containing the +interactive component. Please check your LaTeX to be sure it conforms. +See %\href{https://journals.aas.org/aastexguide/interactivefig}{stuff} +%{https://journals.aas.org/aastexguide/\#interactivefig} +for more details. +\vskip12pt\hrule height1pt \else\global\correctentriestrue\fi +\global\currwidth\hsize +\global\advance\currwidth by -32pt +%% we need to set \currwidth here because interactbox expands +%% before highlightfigure +\global\setbox\interactbox=\vbox\bgroup\hsize=\currwidth\centering} + +\def\endinteractive{\egroup +\ifcorrectentries\highlightfigure{\copy\interactbox}\fi} + diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/bib.bib b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/bib.bib new file mode 100644 index 0000000..be6df26 --- /dev/null +++ b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/bib.bib @@ -0,0 +1,1966 @@ +@ARTICLE{1939ApJKuiper, + author = {{Kuiper}, G.~P.}, + title = "{Two New White Dwarfs; Notes on Proper Motion Stars.}", + journal = {\apj}, + year = 1939, + month = may, + volume = {89}, + pages = {548}, + doi = {10.1086/144075}, + adsurl = {https://ui.adsabs.harvard.edu/abs/1939ApJ....89..548K}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{1940ApJKuiper, + author = {{Kuiper}, G.~P.}, + title = "{New White Dwarfs, Subdwarfs, and Binary Stars.}", + journal = {\apj}, + year = 1940, + month = mar, + volume = {91}, + pages = {269}, + doi = {10.1086/144166}, + adsurl = {https://ui.adsabs.harvard.edu/abs/1940ApJ....91..269K}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2012A&AFontaine, + author = {{Fontaine}, G. and {Brassard}, P. and {Charpinet}, S. and {Green}, E.~M. and {Randall}, S.~K. and {Van Grootel}, V.}, + title = "{A preliminary look at the empirical mass distribution of hot B subdwarf stars}", + journal = {\aap}, + keywords = {stars: fundamental parameters, stars: oscillations, subdwarfs}, + year = 2012, + month = mar, + volume = {539}, + eid = {A12}, + pages = {A12}, + doi = {10.1051/0004-6361/201118220}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2012A&A...539A..12F}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2024MNRASArancibiaRojas, + author = {{Arancibia-Rojas}, Eduardo and {Zorotovic}, Monica and {Vu{\v{c}}kovi{\'c}}, Maja and {Bobrick}, Alexey and {Vos}, Joris and {Piraino-Cerda}, Franco}, + title = "{The mass range of hot subdwarf B stars from MESA simulations}", + journal = {\mnras}, + keywords = {binaries: general, stars: evolution, stars: mass-loss, subdwarfs, Galaxy: evolution, Astrophysics - Solar and Stellar Astrophysics}, + year = 2024, + month = feb, + volume = {527}, + number = {4}, + pages = {11184-11197}, + doi = {10.1093/mnras/stad3891}, +archivePrefix = {arXiv}, + eprint = {2312.09920}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2024MNRAS.52711184A}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2016PASPHeber, + author = {{Heber}, U.}, + title = "{Hot Subluminous Stars}", + journal = {\pasp}, + keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, + year = 2016, + month = aug, + volume = {128}, + number = {966}, + pages = {082001}, + doi = {10.1088/1538-3873/128/966/082001}, +archivePrefix = {arXiv}, + eprint = {1604.07749}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2016PASP..128h2001H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2022A&ACulpan, + author = {{Culpan}, R. and {Geier}, S. and {Reindl}, N. and {Pelisoli}, I. and {Gentile Fusillo}, N. and {Vorontseva}, A.}, + title = "{The population of hot subdwarf stars studied with Gaia. IV. Catalogues of hot subluminous stars based on Gaia EDR3}", + journal = {\aap}, + keywords = {subdwarfs, Hertzsprung-Russell and C-M diagrams, binaries: general, stars: horizontal-branch, catalogs, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, + year = 2022, + month = jun, + volume = {662}, + eid = {A40}, + pages = {A40}, + doi = {10.1051/0004-6361/202243337}, +archivePrefix = {arXiv}, + eprint = {2203.07938}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...662A..40C}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2022ApJGe, + author = {{Ge}, Hongwei and {Tout}, Christopher A. and {Chen}, Xuefei and {Kruckow}, Matthias U. and {Chen}, Hailiang and {Jiang}, Dengkai and {Li}, Zhenwei and {Liu}, Zhengwei and {Han}, Zhanwen}, + title = "{The Common Envelope Evolution Outcome-A Case Study on Hot Subdwarf B Stars}", + journal = {\apj}, + keywords = {Common envelope evolution, Stellar physics, Stellar evolution, Binary stars, 2154, 1621, 1599, 154, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena}, + year = 2022, + month = jul, + volume = {933}, + number = {2}, + eid = {137}, + pages = {137}, + doi = {10.3847/1538-4357/ac75d3}, +archivePrefix = {arXiv}, + eprint = {2205.14256}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...933..137G}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2014MNRASChen, + author = {{Chen}, Hai-Liang and {Woods}, T.~E. and {Yungelson}, L.~R. and {Gilfanov}, M. and {Han}, Zhanwen}, + title = "{Next generation population synthesis of accreting white dwarfs - I. Hybrid calculations using BSE+MESA}", + journal = {\mnras}, + keywords = {binaries: close, stars: evolution, supernovae: general, white dwarfs, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena}, + year = 2014, + month = dec, + volume = {445}, + number = {2}, + pages = {1912-1923}, + doi = {10.1093/mnras/stu1884}, +archivePrefix = {arXiv}, + eprint = {1404.4450}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2014MNRAS.445.1912C}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2020RAAHan, + author = {{Han}, Zhan-Wen and {Ge}, Hong-Wei and {Chen}, Xue-Fei and {Chen}, Hai-Liang}, + title = "{Binary Population Synthesis}", + journal = {Research in Astronomy and Astrophysics}, + keywords = {stars: evolution, star: binaries (including multiple): close, stars: statistics, supernovae: general, galaxies: stellar content, methods: numerical, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena}, + year = 2020, + month = oct, + volume = {20}, + number = {10}, + eid = {161}, + pages = {161}, + doi = {10.1088/1674-4527/20/10/161}, +archivePrefix = {arXiv}, + eprint = {2009.08611}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2020RAA....20..161H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2012NewARWang, + author = {{Wang}, Bo and {Han}, Zhanwen}, + title = "{Progenitors of type Ia supernovae}", + journal = {New Astronomy Reviews}, + keywords = {binaries: general, stars: evolution, supernovae: general, white dwarfs, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena}, + year = 2012, + month = aug, + volume = {56}, + pages = {122-141}, + doi = {10.1016/j.newar.2012.04.001}, +archivePrefix = {arXiv}, + eprint = {1204.4907}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2012NewAR..56..122W}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + + +@ARTICLE{2012MNRASZhang, + author = {{Zhang}, Xianfei and {Jeffery}, C. Simon}, + title = "{Evolutionary models for double helium white dwarf mergers and the formation of helium-rich hot subdwarfs}", + journal = {\mnras}, + keywords = {stars: abundances, binaries: close, stars: evolution, stars: peculiar, subdwarfs, white dwarfs}, + year = 2012, + month = jan, + volume = {419}, + number = {1}, + pages = {452-464}, + doi = {10.1111/j.1365-2966.2011.19711.x}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2012MNRAS.419..452Z}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2020RAAHan, + author = {{Han}, Zhan-Wen and {Ge}, Hong-Wei and {Chen}, Xue-Fei and {Chen}, Hai-Liang}, + title = "{Binary Population Synthesis}", + journal = {Research in Astronomy and Astrophysics}, + keywords = {stars: evolution, star: binaries (including multiple): close, stars: statistics, supernovae: general, galaxies: stellar content, methods: numerical, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena}, + year = 2020, + month = oct, + volume = {20}, + number = {10}, + eid = {161}, + pages = {161}, + doi = {10.1088/1674-4527/20/10/161}, +archivePrefix = {arXiv}, + eprint = {2009.08611}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2020RAA....20..161H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2024arXivHeber, + author = {{Heber}, Ulrich}, + title = "{Hot Subdwarf Stars}", + journal = {arXiv e-prints}, + keywords = {Astrophysics - Solar and Stellar Astrophysics}, + year = 2024, + month = oct, + eid = {arXiv:2410.11663}, + pages = {arXiv:2410.11663}, + doi = {10.48550/arXiv.2410.11663}, +archivePrefix = {arXiv}, + eprint = {2410.11663}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2024arXiv241011663H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2022A&ASchaffenroth, + author = {{Schaffenroth}, V. and {Pelisoli}, I. and {Barlow}, B.~N. and {Geier}, S. and {Kupfer}, T.}, + title = "{Hot subdwarfs in close binaries observed from space. I. Orbital, atmospheric, and absolute parameters, and the nature of their companions}", + journal = {\aap}, + keywords = {binaries: close, subdwarfs, white dwarfs, stars: late-type, stars: horizontal-branch, stars: fundamental parameters, Astrophysics - Solar and Stellar Astrophysics}, + year = 2022, + month = oct, + volume = {666}, + eid = {A182}, + pages = {A182}, + doi = {10.1051/0004-6361/202244214}, +archivePrefix = {arXiv}, + eprint = {2207.02001}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...666A.182S}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2024ApJLi, + author = {{Li}, Zhenwei and {Zhang}, Yangyang and {Chen}, Hailiang and {Ge}, Hongwei and {Jiang}, Dengkai and {Li}, Jiangdan and {Chen}, Xuefei and {Han}, Zhanwen}, + title = "{A New Route to Massive Hot Subdwarfs: Common Envelope Ejection from Asymptotic Giant Branch Stars}", + journal = {\apj}, + keywords = {Subdwarf stars, Common envelope evolution, Asymptotic giant branch, Binary stars, 2054, 2154, 108, 154, Astrophysics - Solar and Stellar Astrophysics}, + year = 2024, + month = mar, + volume = {964}, + number = {1}, + eid = {22}, + pages = {22}, + doi = {10.3847/1538-4357/ad2206}, +archivePrefix = {arXiv}, + eprint = {2401.12429}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2024ApJ...964...22L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2022MNRASLi, + author = {{Li}, Jiangdan and {Onken}, Christopher A. and {Wolf}, Christian and {N{\'e}meth}, P{\'e}ter and {Bessell}, Mike and {Li}, Zhenwei and {Zhang}, Xiaobin and {Li}, Jiao and {Wang}, Luqian and {Li}, Lifang and {Luo}, Yangping and {Chen}, Hailiang and {Ji}, Kaifan and {Chen}, Xuefei and {Han}, Zhanwen}, + title = "{A Roche lobe-filling hot subdwarf and white dwarf binary: possible detection of an ejected common envelope}", + journal = {\mnras}, + keywords = {binaries: close, stars: individual: J192054.50-200135.5, subdwarfs, white dwarfs, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena}, + year = 2022, + month = sep, + volume = {515}, + number = {3}, + pages = {3370-3382}, + doi = {10.1093/mnras/stac1768}, +archivePrefix = {arXiv}, + eprint = {2208.01253}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.515.3370L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2022A&AUzundag, + author = {{Uzundag}, Murat and {Jones}, Mat{\'\i}as I. and {Vu{\v{c}}kovi{\'c}}, Maja and {Vos}, Joris and {Bobrick}, Alexey and {Paladini}, Claudia}, + title = "{Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars. l. Sample selection and binary classification method}", + journal = {\aap}, + keywords = {stars: low-mass, subdwarfs, stars: late-type, binaries: spectroscopic, catalogs, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, + year = 2022, + month = dec, + volume = {668}, + eid = {A89}, + pages = {A89}, + doi = {10.1051/0004-6361/202244638}, +archivePrefix = {arXiv}, + eprint = {2209.08971}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...668A..89U}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2021MNRASYu, + author = {{Yu}, Jinlong and {Zhang}, Xianfei and {L{\"u}}, Guoliang}, + title = "{Post-merger evolution of double helium white dwarfs and distribution of helium-rich hot subdwarfs}", + journal = {\mnras}, + keywords = {binaries: close, stars: fundamental parameters, stars: white dwarfs, Astrophysics - Solar and Stellar Astrophysics}, + year = 2021, + month = jun, + volume = {504}, + number = {2}, + pages = {2670-2674}, + doi = {10.1093/mnras/stab1063}, +archivePrefix = {arXiv}, + eprint = {2104.06817}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.504.2670Y} +} +@ARTICLE{2002MNRASHan, + author = {{Han}, Z. and {Podsiadlowski}, Ph. and {Maxted}, P.~F.~L. and {Marsh}, T.~R. and {Ivanova}, N.}, + title = "{The origin of subdwarf B stars - I. The formation channels}", + journal = {\mnras}, + keywords = {Astrophysics}, + year = 2002, + month = oct, + volume = {336}, + number = {2}, + pages = {449-466}, + doi = {10.1046/j.1365-8711.2002.05752.x}, +archivePrefix = {arXiv}, + eprint = {astro-ph/0206130}, + primaryClass = {astro-ph}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2002MNRAS.336..449H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2003MNRASHan, + author = {{Han}, Z. and {Podsiadlowski}, Ph. and {Maxted}, P.~F.~L. and {Marsh}, T.~R.}, + title = "{The origin of subdwarf B stars - II}", + journal = {\mnras}, + keywords = {binaries: close, subdwarfs, white dwarfs, Astrophysics}, + year = 2003, + month = may, + volume = {341}, + number = {2}, + pages = {669-691}, + doi = {10.1046/j.1365-8711.2003.06451.x}, +archivePrefix = {arXiv}, + eprint = {astro-ph/0301380}, + primaryClass = {astro-ph}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2003MNRAS.341..669H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2022A&AGeier, + author = {{Geier}, S. and {Dorsch}, M. and {Pelisoli}, I. and {Reindl}, N. and {Heber}, U. and {Irrgang}, A.}, + title = "{Radial velocity variability and the evolution of hot subdwarf stars}", + journal = {\aap}, + keywords = {subdwarfs, binaries: spectroscopic, stars: horizontal-branch, Astrophysics - Solar and Stellar Astrophysics}, + year = 2022, + month = may, + volume = {661}, + eid = {A113}, + pages = {A113}, + doi = {10.1051/0004-6361/202143022}, +archivePrefix = {arXiv}, + eprint = {2202.09608}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...661A.113G}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2025SCPMA..6869511L, + author = {{Luo}, Changqing and {Li}, Jiao and {Zheng}, Chuanjie and {Liu}, Dongdong and {Li}, Zhenwei and {Luo}, Yangping and {N{\'e}meth}, P{\'e}ter and {Zhang}, Bo and {Xiong}, Jianping and {Wang}, Bo and {Wang}, Song and {Bai}, Yu and {Li}, Qingzheng and {Wang}, Pei and {Han}, Zhanwen and {Liu}, Jifeng and {Huang}, Yang and {Chen}, Xuefei and {Liu}, Chao}, + title = "{A born ultramassive white dwarf-hot subdwarf super-Chandrasekhar candidate}", + journal = {Science China Physics, Mechanics, and Astronomy}, + keywords = {stars:horizontal branch, subdwarfs, binaries:close, white dwarfs, stars:neutron, supernovae:general, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena}, + year = 2025, + month = jun, + volume = {68}, + number = {6}, + eid = {269511}, + pages = {269511}, + doi = {10.1007/s11433-024-2630-x}, +archivePrefix = {arXiv}, + eprint = {2404.04835}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2025SCPMA..6869511L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + + + +@ARTICLE{2000MNRASHurley, + author = {{Hurley}, Jarrod R. and {Pols}, Onno R. and {Tout}, Christopher A.}, + title = "{Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity}", + journal = {\mnras}, + keywords = {METHODS: ANALYTICAL, STARS: EVOLUTION, STARS: FUNDAMENTAL PARAMETERS, STARS: MASS-LOSS, STARS: POPULATION II, GALAXIES: STELLAR CONTENT, Astrophysics}, + year = 2000, + month = jul, + volume = {315}, + number = {3}, + pages = {543-569}, + doi = {10.1046/j.1365-8711.2000.03426.x}, +archivePrefix = {arXiv}, + eprint = {astro-ph/0001295}, + primaryClass = {astro-ph}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2000MNRAS.315..543H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2017A&AGeier, + author = {{Geier}, S. and {{\O}stensen}, R.~H. and {Nemeth}, P. and {Gentile Fusillo}, N.~P. and {G{\"a}nsicke}, B.~T. and {Telting}, J.~H. and {Green}, E.~M. and {Schaffenroth}, J.}, + title = "{The population of hot subdwarf stars studied with Gaia. I. The catalog of known hot subdwarf stars}", + journal = {\aap}, + keywords = {subdwarfs, stars: horizontal-branch, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, + year = 2017, + month = apr, + volume = {600}, + eid = {A50}, + pages = {A50}, + doi = {10.1051/0004-6361/201630135}, +archivePrefix = {arXiv}, + eprint = {1612.02995}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2017A&A...600A..50G}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{1979ApJSMiller, + author = {{Miller}, G.~E. and {Scalo}, J.~M.}, + title = "{The Initial Mass Function and Stellar Birthrate in the Solar Neighborhood}", + journal = {\apjs}, + keywords = {Cosmology, Solar System, Stellar Evolution, Stellar Mass, Gas Density, Main Sequence Stars, Milky Way Galaxy, Nuclear Fusion, Planetary Nebulae, Stellar Luminosity, Stellar Mass Accretion, Stellar Mass Ejection, Supernovae, White Dwarf Stars, Astrophysics}, + year = 1979, + month = nov, + volume = {41}, + pages = {513}, + doi = {10.1086/190629}, + adsurl = {https://ui.adsabs.harvard.edu/abs/1979Ap} +} + +@ARTICLE{2022ApJZeng, + author = {{Zeng}, Yaotian and {Liu}, Zheng-Wei and {Heger}, Alexander and {McCully}, Curtis and {R{\"o}pke}, Friedrich K. and {Han}, Zhanwen}, + title = "{Long-term Evolution of Postexplosion Helium-star Companions of Type Iax Supernovae}", + journal = {\apj}, + keywords = {Close binary stars, Supernovae, Type Ia supernovae, 254, 1668, 1728, Astrophysics - 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Summary of the contents and survey properties}", + journal = {\aap}, + keywords = {catalogs, astrometry, parallaxes, proper motions, techniques: photometric, techniques: radial velocities, Astrophysics - Astrophysics of Galaxies}, + year = 2021, + month = may, + volume = {649}, + eid = {A1}, + pages = {A1}, + doi = {10.1051/0004-6361/202039657}, +archivePrefix = {arXiv}, + eprint = {2012.01533}, + primaryClass = {astro-ph.GA}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...649A...1G}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2020ApJ...889..117L, + author = {{Lei}, Zhenxin and {Zhao}, Jingkun and {N{\'e}meth}, P{\'e}ter and {Zhao}, Gang}, + title = "{Hot Subdwarf Stars Identified in Gaia DR2 with Spectra of LAMOST DR6 and DR7. I. Single-lined Spectra}", + journal = {\apj}, + keywords = {Subdwarf stars, Stellar classification, Surveys, 2054, 1589, 1671, Astrophysics - Solar and Stellar Astrophysics}, + year = 2020, + month = feb, + volume = {889}, + number = {2}, + eid = {117}, + pages = {117}, + doi = {10.3847/1538-4357/ab660a}, +archivePrefix = {arXiv}, + eprint = {1912.11205}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...889..117L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2019ApJ...881..135L, + author = {{Lei}, Zhenxin and {Zhao}, Jingkun and {N{\'e}meth}, P{\'e}ter and {Zhao}, Gang}, + title = "{New Hot Subdwarf Stars Identified in Gaia DR2 with LAMOST DR5 Spectra. II.}", + journal = {\apj}, + keywords = {subdwarfs, surveys, Astrophysics - Solar and Stellar Astrophysics}, + year = 2019, + month = aug, + volume = {881}, + number = {2}, + eid = {135}, + pages = {135}, + doi = {10.3847/1538-4357/ab2edc}, +archivePrefix = {arXiv}, + eprint = {1907.00128}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...881..135L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + + +@ARTICLE{2019PASJ...71...41L, + author = {{Lei}, Zhenxin and {Bu}, Yude and {Zhao}, Jingkun and {N{\'e}meth}, P{\'e}ter and {Zhao}, Gang}, + title = "{Searching for hot subdwarf stars from the LAMOST Spectra. II. Pure spectroscopic identification method for hot subdwarfs}", + journal = {\pasj}, + keywords = {methods: miscellaneous, subdwarfs, surveys, Astrophysics - Solar and Stellar Astrophysics}, + year = 2019, + month = apr, + volume = {71}, + number = {2}, + eid = {41}, + pages = {41}, + doi = {10.1093/pasj/psz006}, +archivePrefix = {arXiv}, + eprint = {1907.00132}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2019PASJ...71...41L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2021ApJS..256...28L, + author = {{Luo}, Yangping and {N{\'e}meth}, P{\'e}ter and {Wang}, Kun and {Wang}, Xi and {Han}, Zhanwen}, + title = "{Hot Subdwarf Atmospheric Parameters, Kinematics, and Origins Based on 1587 Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR7}", + journal = {\apjs}, + keywords = {O subdwarf stars, Stellar kinematics, 1138, 1608, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, + year = 2021, + month = oct, + volume = {256}, + number = {2}, + eid = {28}, + pages = {28}, + doi = {10.3847/1538-4365/ac11f6}, +archivePrefix = {arXiv}, + eprint = {2107.09302}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJS..256...28L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2019ApJ...881....7L, + author = {{Luo}, Yangping and {N{\'e}meth}, P{\'e}ter and {Deng}, Licai and {Han}, Zhanwen}, + title = "{Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR5}", + journal = {\apj}, + keywords = {stars: kinematics and dynamics, subdwarfs, surveys, Astrophysics - Solar and Stellar Astrophysics}, + year = 2019, + month = aug, + volume = {881}, + number = {1}, + eid = {7}, + pages = {7}, + doi = {10.3847/1538-4357/ab298d}, +archivePrefix = {arXiv}, + eprint = {1906.09393}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...881....7L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2019MNRAS.486.2169K, + author = {{Kepler}, S.~O. and {Pelisoli}, Ingrid and {Koester}, Detlev and {Reindl}, Nicole and {Geier}, Stephan and {Romero}, Alejandra D. and {Ourique}, Gustavo and {Oliveira}, Cristiane de Paula and {Amaral}, Larissa A.}, + title = "{White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 14}", + journal = {\mnras}, + keywords = {catalogues, subdwarfs, white dwarfs; stars: fundamental parameters; cataclysmic variables, Astrophysics - Solar and Stellar Astrophysics}, + year = 2019, + month = jun, + volume = {486}, + number = {2}, + pages = {2169-2183}, + doi = {10.1093/mnras/stz960}, +archivePrefix = {arXiv}, + eprint = {1904.01626}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2169K}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2017OAst...26..164G, + author = {{Geier}, Stephan and {{\O}stensen}, Roy H. and {Nemeth}, Peter and {Heber}, Ulrich and {Gentile Fusillo}, Nicola P. and {G{\"a}nsicke}, Boris T. and {Telting}, John H. and {Green}, Elizabeth M. and {Schaffenroth}, Johannes}, + title = "{Meet the family - the catalog of known hot subdwarf stars}", + journal = {Open Astronomy}, + keywords = {stars: subdwarfs, stars: horizontal branch, catalogs, Astrophysics - Solar and Stellar Astrophysics}, + year = 2017, + month = dec, + volume = {26}, + number = {1}, + pages = {164-168}, + doi = {10.1515/astro-2017-0432}, +archivePrefix = {arXiv}, + eprint = {1711.01856}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2017OAst...26..164G}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2019A&A...630A..80S, + author = {{Schaffenroth}, V. and {Barlow}, B.~N. and {Geier}, S. and {Vu{\v{c}}kovi{\'c}}, M. and {Kilkenny}, D. and {Wolz}, M. and {Kupfer}, T. and {Heber}, U. and {Drechsel}, H. and {Kimeswenger}, S. and {Marsh}, T. and {Wolf}, M. and {Pelisoli}, I. and {Freudenthal}, J. and {Dreizler}, S. and {Kreuzer}, S. and {Ziegerer}, E.}, + title = "{The EREBOS project: Investigating the effect of substellar and low-mass stellar companions on late stellar evolution. Survey, target selection, and atmospheric parameters}", + journal = {\aap}, + keywords = {binaries: eclipsing, brown dwarfs, binaries: spectroscopic, binaries: close, subdwarfs, surveys, Astrophysics - Solar and Stellar Astrophysics}, + year = 2019, + month = oct, + volume = {630}, + eid = {A80}, + pages = {A80}, + doi = {10.1051/0004-6361/201936019}, +archivePrefix = {arXiv}, + eprint = {1907.09892}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2019A&A...630A..80S}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2022A&A...666A.182S, + author = {{Schaffenroth}, V. and {Pelisoli}, I. and {Barlow}, B.~N. and {Geier}, S. and {Kupfer}, T.}, + title = "{Hot subdwarfs in close binaries observed from space. I. Orbital, atmospheric, and absolute parameters, and the nature of their companions}", + journal = {\aap}, + keywords = {binaries: close, subdwarfs, white dwarfs, stars: late-type, stars: horizontal-branch, stars: fundamental parameters, Astrophysics - Solar and Stellar Astrophysics}, + year = 2022, + month = oct, + volume = {666}, + eid = {A182}, + pages = {A182}, + doi = {10.1051/0004-6361/202244214}, +archivePrefix = {arXiv}, + eprint = {2207.02001}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...666A.182S}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2023A&A...673A..90S, + author = {{Schaffenroth}, V. and {Barlow}, B.~N. and {Pelisoli}, I. and {Geier}, S. and {Kupfer}, T.}, + title = "{Hot subdwarfs in close binaries observed from space. II. Analyses of the light variations}", + journal = {\aap}, + keywords = {binaries : close, stars: variables: general, subdwarfs, stars: horizontal-branch, stars: low-mass, stars: fundamental parameters, Astrophysics - Solar and Stellar Astrophysics}, + year = 2023, + month = may, + volume = {673}, + eid = {A90}, + pages = {A90}, + doi = {10.1051/0004-6361/202244697}, +archivePrefix = {arXiv}, + eprint = {2302.12507}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2023A&A...673A..90S}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2021MNRAS.501..623J, + author = {{Jeffery}, C.~S. and {Miszalski}, B. and {Snowdon}, E.}, + title = "{The SALT survey of helium-rich hot subdwarfs: methods, classification, and coarse analysis}", + journal = {\mnras}, + keywords = {surveys, stars: chemically peculiar, stars: early type, stars: fundamental parameters, subdwarfs, Astrophysics - Solar and Stellar Astrophysics}, + year = 2021, + month = feb, + volume = {501}, + number = {1}, + pages = {623-642}, + doi = {10.1093/mnras/staa3648}, +archivePrefix = {arXiv}, + eprint = {2011.09523}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.501..623J}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2015JATIS...1a4003R, + author = {{Ricker}, George R. and {Winn}, Joshua N. and {Vanderspek}, Roland and {Latham}, David W. and {Bakos}, G{\'a}sp{\'a}r {\'A}. and {Bean}, Jacob L. and {Berta-Thompson}, Zachory K. and {Brown}, Timothy M. and {Buchhave}, Lars and {Butler}, Nathaniel R. and {Butler}, R. Paul and {Chaplin}, William J. and {Charbonneau}, David and {Christensen-Dalsgaard}, J{\o}rgen and {Clampin}, Mark and {Deming}, Drake and {Doty}, John and {De Lee}, Nathan and {Dressing}, Courtney and {Dunham}, Edward W. and {Endl}, Michael and {Fressin}, Francois and {Ge}, Jian and {Henning}, Thomas and {Holman}, Matthew J. and {Howard}, Andrew W. and {Ida}, Shigeru and {Jenkins}, Jon M. and {Jernigan}, Garrett and {Johnson}, John Asher and {Kaltenegger}, Lisa and {Kawai}, Nobuyuki and {Kjeldsen}, Hans and {Laughlin}, Gregory and {Levine}, Alan M. and {Lin}, Douglas and {Lissauer}, Jack J. and {MacQueen}, Phillip and {Marcy}, Geoffrey and {McCullough}, Peter R. and {Morton}, Timothy D. and {Narita}, Norio and {Paegert}, Martin and {Palle}, Enric and {Pepe}, Francesco and {Pepper}, Joshua and {Quirrenbach}, Andreas and {Rinehart}, Stephen A. and {Sasselov}, Dimitar and {Sato}, Bun'ei and {Seager}, Sara and {Sozzetti}, Alessandro and {Stassun}, Keivan G. and {Sullivan}, Peter and {Szentgyorgyi}, Andrew and {Torres}, Guillermo and {Udry}, Stephane and {Villasenor}, Joel}, + title = "{Transiting Exoplanet Survey Satellite (TESS)}", + journal = {Journal of Astronomical Telescopes, Instruments, and Systems}, + year = 2015, + month = jan, + volume = {1}, + eid = {014003}, + pages = {014003}, + doi = {10.1117/1.JATIS.1.1.014003}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2015JATIS...1a4003R}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2014PASP..126..398H, + author = {{Howell}, Steve B. and {Sobeck}, Charlie and {Haas}, Michael and {Still}, Martin and {Barclay}, Thomas and {Mullally}, Fergal and {Troeltzsch}, John and {Aigrain}, Suzanne and {Bryson}, Stephen T. and {Caldwell}, Doug and {Chaplin}, William J. and {Cochran}, William D. and {Huber}, Daniel and {Marcy}, Geoffrey W. and {Miglio}, Andrea and {Najita}, Joan R. and {Smith}, Marcie and {Twicken}, J.~D. and {Fortney}, Jonathan J.}, + title = "{The K2 Mission: Characterization and Early Results}", + journal = {\pasp}, + keywords = {Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, + year = 2014, + month = apr, + volume = {126}, + number = {938}, + pages = {398}, + doi = {10.1086/676406}, +archivePrefix = {arXiv}, + eprint = {1402.5163}, + primaryClass = {astro-ph.IM}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2014PASP..126..398H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2012RAA....12.1197C, + author = {{Cui}, Xiang-Qun and {Zhao}, Yong-Heng and {Chu}, Yao-Quan and {Li}, Guo-Ping and {Li}, Qi and {Zhang}, Li-Ping and {Su}, Hong-Jun and {Yao}, Zheng-Qiu and {Wang}, Ya-Nan and {Xing}, Xiao-Zheng and {Li}, Xin-Nan and {Zhu}, Yong-Tian and {Wang}, Gang and {Gu}, Bo-Zhong and {Luo}, A. -Li and {Xu}, Xin-Qi and {Zhang}, Zhen-Chao and {Liu}, Gen-Rong and {Zhang}, Hao-Tong and {Yang}, De-Hua and {Cao}, Shu-Yun and {Chen}, Hai-Yuan and {Chen}, Jian-Jun and {Chen}, Kun-Xin and {Chen}, Ying and {Chu}, Jia-Ru and {Feng}, Lei and {Gong}, Xue-Fei and {Hou}, Yong-Hui and {Hu}, Hong-Zhuan and {Hu}, Ning-Sheng and {Hu}, Zhong-Wen and {Jia}, Lei and {Jiang}, Fang-Hua and {Jiang}, Xiang and {Jiang}, Zi-Bo and {Jin}, Ge and {Li}, Ai-Hua and {Li}, Yan and {Li}, Ye-Ping and {Liu}, Guan-Qun and {Liu}, Zhi-Gang and {Lu}, Wen-Zhi and {Mao}, Yin-Dun and {Men}, Li and {Qi}, Yong-Jun and {Qi}, Zhao-Xiang and {Shi}, Huo-Ming and {Tang}, Zheng-Hong and {Tao}, Qing-Sheng and {Wang}, Da-Qi and {Wang}, Dan and {Wang}, Guo-Min and {Wang}, Hai and {Wang}, Jia-Ning and {Wang}, Jian and {Wang}, Jian-Ling and {Wang}, Jian-Ping and {Wang}, Lei and {Wang}, Shu-Qing and {Wang}, You and {Wang}, Yue-Fei and {Xu}, Ling-Zhe and {Xu}, Yan and {Yang}, Shi-Hai and {Yu}, Yong and {Yuan}, Hui and {Yuan}, Xiang-Yan and {Zhai}, Chao and {Zhang}, Jing and {Zhang}, Yan-Xia and {Zhang}, Yong and {Zhao}, Ming and {Zhou}, Fang and {Zhou}, Guo-Hua and {Zhu}, Jie and {Zou}, Si-Cheng}, + title = "{The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)}", + journal = {Research in Astronomy and Astrophysics}, + year = 2012, + month = sep, + volume = {12}, + number = {9}, + pages = {1197-1242}, + doi = {10.1088/1674-4527/12/9/003}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2012RAA....12.1197C}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2012RAA....12..723Z, + author = {{Zhao}, Gang and {Zhao}, Yong-Heng and {Chu}, Yao-Quan and {Jing}, Yi-Peng and {Deng}, Li-Cai}, + title = "{LAMOST spectral survey {\textemdash} An overview}", + journal = {Research in Astronomy and Astrophysics}, + year = 2012, + month = jul, + volume = {12}, + number = {7}, + pages = {723-734}, + doi = {10.1088/1674-4527/12/7/002}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2012RAA....12..723Z}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2020ApJS..249....3A, + author = {{Ahumada}, Romina and {Allende Prieto}, Carlos and {Almeida}, Andr{\'e}s and {Anders}, Friedrich and {Anderson}, Scott F. and {Andrews}, Brett H. and {Anguiano}, Borja and {Arcodia}, Riccardo and {Armengaud}, Eric and {Aubert}, Marie and {Avila}, Santiago and {Avila-Reese}, Vladimir and {Badenes}, Carles and {Balland}, Christophe and {Barger}, Kat and {Barrera-Ballesteros}, Jorge K. and {Basu}, Sarbani and {Bautista}, Julian and {Beaton}, Rachael L. and {Beers}, Timothy C. and {Benavides}, B. Izamar T. and {Bender}, Chad F. and {Bernardi}, Mariangela and {Bershady}, Matthew and {Beutler}, Florian and {Bidin}, Christian Moni and {Bird}, Jonathan and {Bizyaev}, Dmitry and {Blanc}, Guillermo A. and {Blanton}, Michael R. and {Boquien}, M{\'e}d{\'e}ric and {Borissova}, Jura and {Bovy}, Jo and {Brandt}, W.~N. and {Brinkmann}, Jonathan and {Brownstein}, Joel R. and {Bundy}, Kevin and {Bureau}, Martin and {Burgasser}, Adam and {Burtin}, Etienne and {Cano-D{\'\i}az}, Mariana and {Capasso}, Raffaella and {Cappellari}, Michele and {Carrera}, Ricardo and {Chabanier}, Sol{\`e}ne and {Chaplin}, William and {Chapman}, Michael and {Cherinka}, Brian and {Chiappini}, Cristina and {Doohyun Choi}, Peter and {Chojnowski}, S. Drew and {Chung}, Haeun and {Clerc}, Nicolas and {Coffey}, Damien and {Comerford}, Julia M. and {Comparat}, Johan and {da Costa}, Luiz and {Cousinou}, Marie-Claude and {Covey}, Kevin and {Crane}, Jeffrey D. and {Cunha}, Katia and {Ilha}, Gabriele da Silva and {Dai}, Yu Sophia and {Damsted}, Sanna B. and {Darling}, Jeremy and {Davidson}, Jr., James W. and {Davies}, Roger and {Dawson}, Kyle and {De}, Nikhil and {de la Macorra}, Axel and {De Lee}, Nathan and {Queiroz}, Anna B{\'a}rbara de Andrade and {Deconto Machado}, Alice and {de la Torre}, Sylvain and {Dell'Agli}, Flavia and {du Mas des Bourboux}, H{\'e}lion and {Diamond-Stanic}, Aleksandar M. and {Dillon}, Sean and {Donor}, John and {Drory}, Niv and {Duckworth}, Chris and {Dwelly}, Tom and {Ebelke}, Garrett and {Eftekharzadeh}, Sarah and {Davis Eigenbrot}, Arthur and {Elsworth}, Yvonne P. and {Eracleous}, Mike and {Erfanianfar}, Ghazaleh and {Escoffier}, Stephanie and {Fan}, Xiaohui and {Farr}, Emily and {Fern{\'a}ndez-Trincado}, Jos{\'e} G. and {Feuillet}, Diane and {Finoguenov}, Alexis and {Fofie}, Patricia and {Fraser-McKelvie}, Amelia and {Frinchaboy}, Peter M. and {Fromenteau}, Sebastien and {Fu}, Hai and {Galbany}, Llu{\'\i}s and {Garcia}, Rafael A. and {Garc{\'\i}a-Hern{\'a}ndez}, D.~A. and {Garma Oehmichen}, Luis Alberto and {Ge}, Junqiang and {Geimba Maia}, Marcio Antonio and {Geisler}, Doug and {Gelfand}, Joseph and {Goddy}, Julian and {Gonzalez-Perez}, Violeta and {Grabowski}, Kathleen and {Green}, Paul and {Grier}, Catherine J. and {Guo}, Hong and {Guy}, Julien and {Harding}, Paul and {Hasselquist}, Sten and {Hawken}, Adam James and {Hayes}, Christian R. and {Hearty}, Fred and {Hekker}, S. and {Hogg}, David W. and {Holtzman}, Jon A. and {Horta}, Danny and {Hou}, Jiamin and {Hsieh}, Bau-Ching and {Huber}, Daniel and {Hunt}, Jason A.~S. and {Ider Chitham}, J. and {Imig}, Julie and {Jaber}, Mariana and {Jimenez Angel}, Camilo Eduardo and {Johnson}, Jennifer A. and {Jones}, Amy M. and {J{\"o}nsson}, Henrik and {Jullo}, Eric and {Kim}, Yerim and {Kinemuchi}, Karen and {Kirkpatrick}, IV, Charles C. and {Kite}, George W. and {Klaene}, Mark and {Kneib}, Jean-Paul and {Kollmeier}, Juna A. and {Kong}, Hui and {Kounkel}, Marina and {Krishnarao}, Dhanesh and {Lacerna}, Ivan and {Lan}, Ting-Wen and {Lane}, Richard R. and {Law}, David R. and {Le Goff}, Jean-Marc and {Leung}, Henry W. and {Lewis}, Hannah and {Li}, Cheng and {Lian}, Jianhui and {Lin}, Lihwai and {Long}, Dan and {Longa-Pe{\~n}a}, Pen{\'e}lope and {Lundgren}, Britt and {Lyke}, Brad W. and {Mackereth}, J. Ted and {MacLeod}, Chelsea L. and {Majewski}, Steven R. and {Manchado}, Arturo and {Maraston}, Claudia and {Martini}, Paul and {Masseron}, Thomas and {Masters}, Karen L. and {Mathur}, Savita and {McDermid}, Richard M. and {Merloni}, Andrea and {Merrifield}, Michael and {M{\'e}sz{\'a}ros}, Szabolcs and {Miglio}, Andrea and {Minniti}, Dante and {Minsley}, Rebecca and {Miyaji}, Takamitsu and {Mohammad}, Faizan Gohar and {Mosser}, Benoit and {Mueller}, Eva-Maria and {Muna}, Demitri and {Mu{\~n}oz-Guti{\'e}rrez}, Andrea and {Myers}, Adam D. and {Nadathur}, Seshadri and {Nair}, Preethi and {Nandra}, Kirpal and {Correa do Nascimento}, Janaina and {Nevin}, Rebecca Jean and {Newman}, Jeffrey A. and {Nidever}, David L. and {Nitschelm}, Christian and {Noterdaeme}, Pasquier and {O'Connell}, Julia E. and {Olmstead}, Matthew D. and {Oravetz}, Daniel and {Oravetz}, Audrey and {Osorio}, Yeisson and {Pace}, Zachary J. and {Padilla}, Nelson and {Palanque-Delabrouille}, Nathalie and {Palicio}, Pedro A.}, + title = "{The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra}", + journal = {\apjs}, + keywords = {Astronomy databases, Optical telescopes, Infrared astronomy, Redshift surveys, Galactic abundances, Stellar spectral lines, Stellar properties, 83, 1174, 786, 1378, 2002, 1630, 1624, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, + year = 2020, + month = jul, + volume = {249}, + number = {1}, + eid = {3}, + pages = {3}, + doi = {10.3847/1538-4365/ab929e}, +archivePrefix = {arXiv}, + eprint = {1912.02905}, + primaryClass = {astro-ph.GA}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJS..249....3A}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2008A&A...491..253M, + author = {{Miller Bertolami}, M.~M. and {Althaus}, L.~G. and {Unglaub}, K. and {Weiss}, A.}, + title = "{Modeling He-rich subdwarfs through the hot-flasher scenario}", + journal = {\aap}, + keywords = {stars: evolution, stars: horizontal-branch, stars: subdwarfs, stars: mass-loss, Astrophysics}, + year = 2008, + month = nov, + volume = {491}, + number = {1}, + pages = {253-265}, + doi = {10.1051/0004-6361:200810373}, +archivePrefix = {arXiv}, + eprint = {0808.3580}, + primaryClass = {astro-ph}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2008A&A...491..253M}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{1993ApJ...407..649C, + author = {{Castellani}, M. and {Castellani}, V.}, + title = "{Mass Loss in Globular Cluster Red Giants: an Evolutionary Investigation}", + journal = {\apj}, + keywords = {Globular Clusters, Red Giant Stars, Stellar Evolution, Stellar Mass Ejection, White Dwarf Stars, Cooling, Stellar Luminosity, Stellar Models, Astrophysics, STARS: EVOLUTION, STARS: MASS LOSS, GALAXY: GLOBULAR CLUSTERS: GENERAL, NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES, STARS: INTERIORS, STARS: POPULATION II}, + year = 1993, + month = apr, + volume = {407}, + pages = {649}, + doi = {10.1086/172547}, + adsurl = {https://ui.adsabs.harvard.edu/abs/1993ApJ...407..649C}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2013A&A...551A..31D, + author = {{Drilling}, J.~S. and {Jeffery}, C.~S. and {Heber}, U. and {Moehler}, S. and {Napiwotzki}, R.}, + title = "{An MK-like system of spectral classification for hot subdwarfs}", + journal = {\aap}, + keywords = {stars: early-type, subdwarfs, stars: atmospheres}, + year = 2013, + month = mar, + volume = {551}, + eid = {A31}, + pages = {A31}, + doi = {10.1051/0004-6361/201219433}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2013A&A...551A..31D}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2024PASJ...76.1084Z, + author = {{Zou}, Xuan and {Lei}, Zhenxin}, + title = "{MK-like spectral classification for hot subdwarf stars with LAMOST spectra}", + journal = {\pasj}, + keywords = {Astrophysics - Solar and Stellar Astrophysics}, + year = 2024, + month = oct, + volume = {76}, + number = {5}, + pages = {1084-1097}, + doi = {10.1093/pasj/psae072}, +archivePrefix = {arXiv}, + eprint = {2407.17062}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2024PASJ...76.1084Z}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2023ApJ...942..109L, + author = {{Lei}, Zhenxin and {He}, Ruijie and {N{\'e}meth}, P{\'e}ter and {Vos}, Joris and {Zou}, Xuan and {Hu}, Ke and {Xiao}, Huaping and {Yan}, Huahui and {Zhao}, Jingkun}, + title = "{Hot Subdwarf Stars Identified in LAMOST DR8 with Single-lined and Composite Spectra}", + journal = {\apj}, + keywords = {B subdwarf stars, Wide binary stars, 129, 1801, Astrophysics - Solar and Stellar Astrophysics}, + year = 2023, + month = jan, + volume = {942}, + number = {2}, + eid = {109}, + pages = {109}, + doi = {10.3847/1538-4357/aca542}, +archivePrefix = {arXiv}, + eprint = {2211.12323}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2023ApJ...942..109L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2025PASA...42...12R, + author = {{Rodr{\'\i}guez-Segovia}, Nicol{\'a}s and {Ruiter}, Ashley J. and {Seitenzahl}, Ivo R.}, + title = "{Population synthesis of hot-subdwarf B stars with COMPAS: Parameter variations and a prescription for hydrogen-rich shells}", + journal = {\pasa}, + keywords = {B subdwarf stars, binary stars, Astrophysics - Solar and Stellar Astrophysics}, + year = 2025, + month = dec, + volume = {42}, + eid = {e012}, + pages = {e012}, + doi = {10.1017/pasa.2024.135}, +archivePrefix = {arXiv}, + eprint = {2412.11712}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2025PASA...42...12R}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2012ApJ...746..186C, + author = {{Clausen}, Drew and {Wade}, Richard A. and {Kopparapu}, Ravi Kumar and {O'Shaughnessy}, Richard}, + title = "{Population Synthesis of Hot Subdwarfs: A Parameter Study}", + journal = {\apj}, + keywords = {binaries: close, stars: horizontal-branch, subdwarfs, Astrophysics - Solar and Stellar Astrophysics}, + year = 2012, + month = feb, + volume = {746}, + number = {2}, + eid = {186}, + pages = {186}, + doi = {10.1088/0004-637X/746/2/186}, +archivePrefix = {arXiv}, + eprint = {1201.0012}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2012ApJ...746..186C}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2012MNRAS.419..452Z, + author = {{Zhang}, Xianfei and {Jeffery}, C. 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Parallax bias versus magnitude, colour, and position}", + journal = {\aap}, + keywords = {astrometry, parallaxes, methods: data analysis, space vehicles: instruments, stars: distances, Astrophysics - Instrumentation and Methods for Astrophysics}, + year = 2021, + month = may, + volume = {649}, + eid = {A4}, + pages = {A4}, + doi = {10.1051/0004-6361/202039653}, +archivePrefix = {arXiv}, + eprint = {2012.01742}, + primaryClass = {astro-ph.IM}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...649A...4L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{1998ApJ...500..525S, + author = {{Schlegel}, David J. and {Finkbeiner}, Douglas P. and {Davis}, Marc}, + title = "{Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds}", + journal = {\apj}, + keywords = {COSMOLOGY: DIFFUSE RADIATION, COSMOLOGY: COSMIC MICROWAVE BACKGROUND, ISM: DUST, EXTINCTION, INTERPLANETARY MEDIUM, INFRARED: ISM: CONTINUUM, Cosmology: Cosmic Microwave Background, Cosmology: Diffuse Radiation, ISM: Dust, Extinction, Infrared: ISM: Continuum, Interplanetary Medium, Astrophysics}, + year = 1998, + month = jun, + volume = {500}, + number = {2}, + pages = {525-553}, + doi = {10.1086/305772}, +archivePrefix = {arXiv}, + eprint = {astro-ph/9710327}, + primaryClass = {astro-ph}, + adsurl = {https://ui.adsabs.harvard.edu/abs/1998ApJ...500..525S}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2011ApJ...737..103S, + author = {{Schlafly}, Edward F. and {Finkbeiner}, Douglas P.}, + title = "{Measuring Reddening with Sloan Digital Sky Survey Stellar Spectra and Recalibrating SFD}", + journal = {\apj}, + keywords = {dust, extinction, Galaxy: stellar content, ISM: clouds, Astrophysics - Galaxy Astrophysics}, + year = 2011, + month = aug, + volume = {737}, + number = {2}, + eid = {103}, + pages = {103}, + doi = {10.1088/0004-637X/737/2/103}, +archivePrefix = {arXiv}, + eprint = {1012.4804}, + primaryClass = {astro-ph.GA}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2011ApJ...737..103S}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@INPROCEEDINGS{2014ASPC..481...95N, + author = {{Nemeth}, P. and {{\"O}stensen}, R. and {Tremblay}, P. and {Hubeny}, I.}, + title = "{Synthetic Spectra for O and B Type Subdwarf Stars}", + keywords = {Astrophysics - Solar and Stellar Astrophysics}, + booktitle = {6th Meeting on Hot Subdwarf Stars and Related Objects}, + year = 2014, + editor = {{van Grootel}, V. and {Green}, E. and {Fontaine}, G. and {Charpinet}, S.}, + series = {Astronomical Society of the Pacific Conference Series}, + volume = {481}, + month = apr, + pages = {95}, + doi = {10.48550/arXiv.1308.0252}, +archivePrefix = {arXiv}, + eprint = {1308.0252}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2014ASPC..481...95N}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{2025MNRAS.539.3273R, + author = {{Rodr{\'\i}guez-Segovia}, Nicol{\'a}s and {Ruiter}, Ashley J.}, + title = "{Population synthesis of hot subdwarf B stars with COMPAS: on the observed Galactic population}", + journal = {\mnras}, + keywords = {binaries: general, stars: statistics, subdwarfs, Solar and Stellar Astrophysics}, + year = 2025, + month = jun, + volume = {539}, + number = {4}, + pages = {3273-3284}, + doi = {10.1093/mnras/staf710}, +archivePrefix = {arXiv}, + eprint = {2505.05791}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2025MNRAS.539.3273R}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{1984ApJ...277..355W, + author = {{Webbink}, R.~F.}, + title = "{Double white dwarfs as progenitors of R Coronae Borealis stars and type I supernovae.}", + journal = {\apj}, + keywords = {Binary Stars, Corona Borealis Constellation, R Coronae Borealis Stars, Stellar Evolution, Supernovae, White Dwarf Stars, B Stars, Carbon Stars, Chandrasekhar Equation, O Stars, Stellar Mass Accretion, Stellar Mass Ejection, Astrophysics}, + year = 1984, + month = feb, + volume = {277}, + pages = {355-360}, + doi = {10.1086/161701}, + adsurl = {https://ui.adsabs.harvard.edu/abs/1984ApJ...277..355W}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{1999PASP..111...63F, + author = {{Fitzpatrick}, Edward L.}, + title = "{Correcting for the Effects of Interstellar Extinction}", + journal = {\pasp}, + keywords = {ISM: DUST, EXTINCTION, Astrophysics}, + year = 1999, + month = jan, + volume = {111}, + number = {755}, + pages = {63-75}, + doi = {10.1086/316293}, +archivePrefix = {arXiv}, + eprint = {astro-ph/9809387}, + primaryClass = {astro-ph}, + adsurl = {https://ui.adsabs.harvard.edu/abs/1999PASP..111...63F}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + +@ARTICLE{1990ApJS...72..163F, + author = {{Fitzpatrick}, Edward L. and {Massa}, Derck}, + title = "{An Analysis of the Shapes of Ultraviolet Extinction Curves. III. an Atlas of Ultraviolet Extinction Curves}", + journal = {\apjs}, + keywords = {Interstellar Extinction, Spectrum Analysis, Stellar Spectra, Ultraviolet Astronomy, Abundance, Astronomical Maps, Astronomical Spectroscopy, H I Regions, Iue, Astrophysics, INTERSTELLAR: ABUNDANCES, INTERSTELLAR: MATTER, ULTRAVIOLET: SPECTRA}, + year = 1990, + month = jan, + volume = {72}, + pages = {163}, + doi = {10.1086/191413}, + adsurl = {https://ui.adsabs.harvard.edu/abs/1990ApJS...72..163F}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + + + +@ARTICLE{2026ApJS..283...16L, + author = {{Lei}, Zhenxin and {Dong}, Yangyang and {Kou}, Bokai and {Feng}, Mengqi and {Hu}, Ke and {Bu}, Yude and {Zhao}, Jingkun}, + title = "{Deep Learning─driven Atmospheric Parameter Prediction for Hot Subdwarf Stars with Synthetic and Observed Spectra}", + journal = {\apjs}, + keywords = {B subdwarf stars, 129, Solar and Stellar Astrophysics}, + year = 2026, + month = mar, + volume = {283}, + number = {1}, + eid = {16}, + pages = {16}, + doi = {10.3847/1538-4365/ae374f}, +archivePrefix = {arXiv}, + eprint = {2512.20185}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2026ApJS..283...16L}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + + + +@ARTICLE{2025A&A...693A.121H, + author = {{He}, Ruijie and {Meng}, Xiangcun and {Lei}, Zhenxin and {Yan}, Huahui and {Lan}, Shunyi}, + title = "{Radial velocity variability fractions of different types of hot subdwarf stars}", + journal = {\aap}, + keywords = {binaries: close, stars: evolution, subdwarfs, Astrophysics - Solar and Stellar Astrophysics}, + year = 2025, + month = jan, + volume = {693}, + eid = {A121}, + pages = {A121}, + doi = {10.1051/0004-6361/202451411}, +archivePrefix = {arXiv}, + eprint = {2412.13963}, + primaryClass = {astro-ph.SR}, + adsurl = {https://ui.adsabs.harvard.edu/abs/2025A&A...693A.121H}, + adsnote = {Provided by the SAO/NASA Astrophysics Data System} +} + + + diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/distribute_mass_spclass.pdf b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/distribute_mass_spclass.pdf new file mode 100644 index 0000000..3629e6c Binary files /dev/null and b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/distribute_mass_spclass.pdf differ diff --git a/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/natbib.sty b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/natbib.sty new file mode 100644 index 0000000..3a355ad --- /dev/null +++ b/Neural_network_based_calculation_of_physical_parameters_of_hot_subdwarfs/natbib.sty @@ -0,0 +1,835 @@ +%% +%% This is file `natbib.sty', +%% generated with the docstrip utility. +%% +%% The original source files were: +%% +%% natbib.dtx (with options: `package,all') +%% ============================================= +%% IMPORTANT NOTICE: +%% +%% This program can be redistributed and/or modified under the terms +%% of the LaTeX Project Public License Distributed from CTAN +%% archives in directory macros/latex/base/lppl.txt; either +%% version 1 of the License, or any later version. +%% +%% This is a generated file. +%% It may not be distributed without the original source file natbib.dtx. +%% +%% Full documentation can be obtained by LaTeXing that original file. +%% Only a few abbreviated comments remain here to describe the usage. +%% ============================================= +%% Copyright 1993-2006 Patrick W Daly +%% Max-Planck-Institut f\"ur Sonnensystemforschung +%% Max-Planck-Str. 2 +%% D-37191 Katlenburg-Lindau +%% Germany +%% E-mail: daly@linmpi.mpg.de +\NeedsTeXFormat{LaTeX2e}[1995/06/01] +\ProvidesPackage{natbib} + [2006/03/22 7.3 (PWD)] + % This package reimplements the LaTeX \cite command to be used for various + % citation styles, both author-year and numerical. It accepts BibTeX + % output intended for many other packages, and therefore acts as a + % general, all-purpose citation-style interface. + % + % With standard numerical .bst files, only numerical citations are + % possible. With an author-year .bst file, both numerical and + % author-year citations are possible. + % + % If author-year citations are selected, \bibitem must have one of the + % following forms: + % \bibitem[Jones et al.(1990)]{key}... + % \bibitem[Jones et al.(1990)Jones, Baker, and Williams]{key}... + % \bibitem[Jones et al., 1990]{key}... + % \bibitem[\protect\citeauthoryear{Jones, Baker, and Williams}{Jones + % et al.}{1990}]{key}... + % \bibitem[\protect\citeauthoryear{Jones et al.}{1990}]{key}... + % \bibitem[\protect\astroncite{Jones et al.}{1990}]{key}... + % \bibitem[\protect\citename{Jones et al., }1990]{key}... + % \harvarditem[Jones et al.]{Jones, Baker, and Williams}{1990}{key}... + % + % This is either to be made up manually, or to be generated by an + % appropriate .bst file with BibTeX. + % Author-year mode || Numerical mode + % Then, \citet{key} ==>> Jones et al. (1990) || Jones et al. [21] + % \citep{key} ==>> (Jones et al., 1990) || [21] + % Multiple citations as normal: + % \citep{key1,key2} ==>> (Jones et al., 1990; Smith, 1989) || [21,24] + % or (Jones et al., 1990, 1991) || [21,24] + % or (Jones et al., 1990a,b) || [21,24] + % \cite{key} is the equivalent of \citet{key} in author-year mode + % and of \citep{key} in numerical mode + % Full author lists may be forced with \citet* or \citep*, e.g. + % \citep*{key} ==>> (Jones, Baker, and Williams, 1990) + % Optional notes as: + % \citep[chap. 2]{key} ==>> (Jones et al., 1990, chap. 2) + % \citep[e.g.,][]{key} ==>> (e.g., Jones et al., 1990) + % \citep[see][pg. 34]{key}==>> (see Jones et al., 1990, pg. 34) + % (Note: in standard LaTeX, only one note is allowed, after the ref. + % Here, one note is like the standard, two make pre- and post-notes.) + % \citealt{key} ==>> Jones et al. 1990 + % \citealt*{key} ==>> Jones, Baker, and Williams 1990 + % \citealp{key} ==>> Jones et al., 1990 + % \citealp*{key} ==>> Jones, Baker, and Williams, 1990 + % Additional citation possibilities (both author-year and numerical modes) + % \citeauthor{key} ==>> Jones et al. + % \citeauthor*{key} ==>> Jones, Baker, and Williams + % \citeyear{key} ==>> 1990 + % \citeyearpar{key} ==>> (1990) + % \citetext{priv. comm.} ==>> (priv. comm.) + % Note: full author lists depends on whether the bib style supports them; + % if not, the abbreviated list is printed even when full requested. + % + % For names like della Robbia at the start of a sentence, use + % \Citet{dRob98} ==>> Della Robbia (1998) + % \Citep{dRob98} ==>> (Della Robbia, 1998) + % \Citeauthor{dRob98} ==>> Della Robbia + % + % + % Citation aliasing is achieved with + % \defcitealias{key}{text} + % \citetalias{key} ==>> text + % \citepalias{key} ==>> (text) + % + % Defining the citation style of a given bib style: + % Use \bibpunct (in the preamble only) with 6 mandatory arguments: + % 1. opening bracket for citation + % 2. closing bracket + % 3. citation separator (for multiple citations in one \cite) + % 4. the letter n for numerical styles, s for superscripts + % else anything for author-year + % 5. punctuation between authors and date + % 6. punctuation between years (or numbers) when common authors missing + % One optional argument is the character coming before post-notes. It + % appears in square braces before all other arguments. May be left off. + % Example (and default) \bibpunct[, ]{(}{)}{;}{a}{,}{,} + % + % To make this automatic for a given bib style, named newbib, say, make + % a local configuration file, natbib.cfg, with the definition + % \newcommand{\bibstyle@newbib}{\bibpunct...} + % Then the \bibliographystyle{newbib} will cause \bibstyle@newbib to + % be called on THE NEXT LATEX RUN (via the aux file). + % + % Such preprogrammed definitions may be invoked in the text (preamble only) + % by calling \citestyle{newbib}. This is only useful if the style specified + % differs from that in \bibliographystyle. + % + % With \citeindextrue and \citeindexfalse, one can control whether the + % \cite commands make an automatic entry of the citation in the .idx + % indexing file. For this, \makeindex must also be given in the preamble. + % + % Package Options: (for selecting punctuation) + % round - round parentheses are used (default) + % square - square brackets are used [option] + % curly - curly braces are used {option} + % angle - angle brackets are used