37 lines
4.2 KiB
TeX
37 lines
4.2 KiB
TeX
\relax
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\@writefile{toc}{\contentsline {section}{\numberline {1}Introduction}{2}{}\protected@file@percent }
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\newlabel{intro}{{1}{2}}
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\newlabel{flux}{{2}{2}}
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\@writefile{toc}{\contentsline {section}{\numberline {2}Installing}{2}{}\protected@file@percent }
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\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Here's your first spectrum with synple. You have modeled the solar spectrum in the vicinity of the Ca I $\lambda $6162 line. The Ca I line is the strong line at the center, visibly damped by collisions with hydrogen atoms. }}{3}{}\protected@file@percent }
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\newlabel{first}{{1}{3}}
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\@writefile{toc}{\contentsline {section}{\numberline {3}Examples}{3}{}\protected@file@percent }
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\@writefile{toc}{\contentsline {subsection}{\numberline {3.1}Computing your first solar spectrum}{3}{}\protected@file@percent }
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\newlabel{6162}{{3.1}{3}}
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\@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces Repeating the calculation in Fig 3.1\hbox {} (blue) but adding a second curve (orange) on the left panel reducing the micro-turbulence from 2 to 1 km s$^{-1}$, and on the right-hand panel increasen the Ca abundance by 0.2 dex. }}{4}{}\protected@file@percent }
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\newlabel{micro-abu}{{2}{4}}
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\@writefile{toc}{\contentsline {subsection}{\numberline {3.2}Altering micro-turbulence and chemical composition}{4}{}\protected@file@percent }
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\newlabel{abundances}{{3.2}{4}}
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\@writefile{lof}{\contentsline {figure}{\numberline {3}{\ignorespaces Repeating the calculation in Fig 3.1\hbox {} (blue) but adding the result of a convolution with a rotational profile for $v \sin i = 5$ km s$^{-1}$ (orange), a Gaussian kernel with a FWHM of 0.2 \r A\ (green), and both (brown). }}{5}{}\protected@file@percent }
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\newlabel{convolution}{{3}{5}}
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\@writefile{toc}{\contentsline {subsection}{\numberline {3.3}Additional line broadening}{5}{}\protected@file@percent }
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\newlabel{fwhm}{{3.3}{5}}
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\@writefile{lof}{\contentsline {figure}{\numberline {4}{\ignorespaces In addition to the original calculation in Fig. 3.1\hbox {} (blue line), we show the result of the convolution with a rotational profile for $v \sin i = 5$ km s$^{-1}$ and a Gaussian kernel with a FWHM of 0.2 \r A\ using {\tt rotconv}{\tt lgconv} (green) and rotin (orange). }}{6}{}\protected@file@percent }
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\newlabel{rotin}{{4}{6}}
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\@writefile{lof}{\contentsline {figure}{\numberline {5}{\ignorespaces We now use all the models in the 'modeldir' directory in one command, with multiple values of the micro, using {\tt multisyn}. }}{7}{}\protected@file@percent }
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\newlabel{rotin}{{5}{7}}
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\@writefile{toc}{\contentsline {subsection}{\numberline {3.4}Multiple models}{7}{}\protected@file@percent }
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\@writefile{lof}{\contentsline {figure}{\numberline {6}{\ignorespaces The main transitions in the spectrum can be labeled activating the {\tt tag} keyword in {\tt syn}. }}{8}{}\protected@file@percent }
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\newlabel{tagging}{{6}{8}}
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\@writefile{toc}{\contentsline {section}{\numberline {4}Identification of spectral features}{8}{}\protected@file@percent }
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\newlabel{tag}{{4}{8}}
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\@writefile{toc}{\contentsline {section}{\numberline {5}Grid handling}{9}{}\protected@file@percent }
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\@writefile{toc}{\contentsline {section}{\numberline {6}Computing opacity tables}{9}{}\protected@file@percent }
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\@writefile{lof}{\contentsline {figure}{\numberline {7}{\ignorespaces Opacity in the range 6100--6110. \r A\ for four combinations of a pair of densities ($\log _{10} \rho = -32.236191, -29.933606$) and temperatures ($\log _{10} T = 8.059055, 8.51957$) and solar abundances. }}{10}{}\protected@file@percent }
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\newlabel{opacity-fig}{{7}{10}}
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\@writefile{toc}{\contentsline {section}{\numberline {7}Computing emergent intensities $I_{\lambda }$}{10}{}\protected@file@percent }
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\@writefile{lof}{\contentsline {figure}{\numberline {8}{\ignorespaces Example of the computation of emergent specific intensities I$_{\lambda }$ for various directions ($\mu = \cos \theta = 1$ the highest and $\mu = \cos \theta = 0.0001$ the lowest). The units are in erg cm$^{-2}$ s$^{-1}$ \r A$^{-1}$ steradian$^{-1}$. }}{11}{}\protected@file@percent }
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\newlabel{intensity-fig}{{8}{11}}
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\@writefile{toc}{\contentsline {section}{\numberline {8}References}{11}{}\protected@file@percent }
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\gdef \@abspage@last{11}
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