kap_data.tar.bz2 This is a tarball, and should be distributed as it is now. It contains OP and OPAL opacity tables adapted to the Asplund et al. (2005, in Astronomical Society of the Pacific Conference Series, Vol. 336, Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, ed. T. G. Barnes III & F. N. Bash, 25) and Cunha et al. (2006ApJ...647L.143C) Ne abundance (A05+Ne), Asplund et al. 2009 (ARA&A, 47, 481 (A09)), and Nieva & Przybilla (2012A&A...539A.143N, Cat. J/A+A/539/A143) and Przybilla et al. (2013, in EAS Publications Series, Vol. 63, EAS Publications Series, 13-23 (NP12)) mixtures. They have to be used with a standard MESA composition option initial_zfracs = 5, 6 8, respectively. All tables are MESA compatible. When querying the OP and OPAL servers, we made a choice to redistribute the abundance residuals on all metals, based on their relative mass fraction instead of depositing them on the heaviest metals, which are Fe and Ni. This is a choice and may slightly influence the adiabatic and non-adiabatic results. These opacity tables fully comply with the MESA standard, and should not be extracted. For a proper installation, they should be placed in the /kap/ (where is the full path to the local MESA installation directory), and then execute the following command in the command prompt: $> ./build_data_and_export inlist, inlist_general, inlist_zoom These files are Fortran 90 free-format Namelists, and are used for the specific setup of our problem, and how evolutionary models were computed These inlists are compatible with MESA version 5548, and the reproducibility of the results is only guaranteed using this specific version gyre3.dat This file is a Fortran 90 free-format Namelist, and is used for the specifying the GYRE computation scheme for adiabatic and non-adiabatic mode resolution. This inlist is compatible with GYRE version 3.0 to 3.2.2 For a more detailed information, you can refer to https://bitbucket.org/rhdtownsend/gyre/wiki/Namelist%20Input%20Files%20(3.0)