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The directory contains input data for computing two opacity tables:
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1) optab11_7f - full table with opacities of all species;
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2) optab11_7hmc - a partial opacity table where the opacity of H, Mg, and Ca
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is removed.
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In both cases, the table has 100,000 wavelength points between 900 and 110,000 A,
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for 11 temperatures between 3 and 15 kK (spaced logarithmicall),
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and 7 densities, between 1.e-12 and 1.e-6 g cm^-3 (again spaced logarithmically).
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In this particular case, the resulting opacity tables optab11_7f.dat and
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optab11_7hmc.dat were not copied to the subderectory results because they
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can be downloaded separately, as explained in Paper IV
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The script R1 runs both test cases, however it is time-consuming, taking
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about 26 and 45 minutes on iMac 3.4GHz for the two respective tables.
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The input data assume that the binary line lists are being used, so that
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they must exist. In the case the binary lists are not used, the user
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should make links to the ASCII files, and to make corresponding changes in
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the files *.3, e.g.
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'gfATO.dat' 0
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'gfMOL.dat' 0 8000.
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'gfTiO.dat' 0 5000.
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In this case, another possibility would be to link the three line lists
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to fort.19 (atomic list), fort.20, and fort.21, delete the fort.3 file,
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and to modify the file fort.55 by adding the last line that sets the
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number of molercular line lists to 2, having unit numbers 20 and 21.
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-3 1 0
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1 0 0 0
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0 0 0 0 0
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1 0 0 0 0
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0 0 0
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900. -110000. 50.00 2000.0 1.00000e-4 0.05
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2 20 21
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If one intends to compute an opacity tables to be used for cool
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(K and M) stars, one should modify the fort.3 file as,
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assuming that one has the binary lists
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'gfATO.bin' 1
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'gfMOL.bin' 1 8000.
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'gfTiO.bin' 1 5000.
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'gfH2O.bin' 1 4000.
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The file gfH2O.dat is available upon request, and the user may
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easily create a binary file using program LIST2BIN.
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