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This archive contains the opacity table of Semenov et al. 2003 as a FORTRAN 77 code. The most important features of the model are overviewed in the header of the code "opacity.f". In addition, an excessive description of its structure as well as an information how to use it are given there. Enjoy! PS. If you have any comments and/or suggestions, please contact me by E-mail. Dmitry Semenov, AIU Jena, March 2003 E-mail: dima@astro.uni-jena.de ------------------------------------------------------------------------------ The 'converter.py' script runs the opacity calculation tool several times and assembles its output into a HDF5 file as a single function on the lg(rho)-lg(T) grid. Evgeny P. Kurbatov, INASAN, Moscow, March 2020 E-mail: evgeny.p.kurbatov@gmail.com, kurbatov@inasan.ru
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Gas and dust opacities for protoplanetary disk calculation
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