The MESA models used in in the paper "Internal mixing of rotating stars inferred from dipole gravity modes" by Pedersen et al. (2021) were computed using MESA version 12115 and the associated GYRE version. ============================================================ Opacity tables ============================================================ The models use a non-standard set of opacity tables included in the directory "KapDataNew". The contents of this directory have to be copied to $MESA_DIR/data/kap_data/, otherwise the included MESA setup will not work. ============================================================ MESA setup ============================================================ The MESA_setup/src directory includes two input files "Dmix_shear.dat" and "Dmix_shear_meridional.dat" which are used to include envelope mixing from vertical shear and meridional circulation including vertical shear, respectively. If either of these profiles are used as a part of a publication, then a reference to George et al. (2013), Astronomy & Astrophysics, Volume 553, id.A24, 17 pp. should be made. Prior to running MESA, the paths to these two files have to be set appropriately in the MESA_setup/src/run_star_extras.f file. In other words, the following lines would have to be modified: character (len=*), PARAMETER :: FileNameShear = & '/your_path/MESA_setup/src/Dmix_shear.dat' character (len=*), PARAMETER :: FileNameShearMeridional = & '/your_path/MESA_setup/src/Dmix_shear_meridional.dat' Finally, the MESA_setup/rn and MESA_setup/src/run_star_extras.f files have been setup such that the varied parameters and choice of mixing profile is set using command line prompts. As an example, to run the MESA inlists for a 5Msun star with convective penetration with alpha_pen = 0.2, a constant envelope mixing with logD_ext = 2, and a metallicity of Z = 0.014, you would run ./rn inlist --logsdir LOGS --initial_mass 5.0 --initial_z 0.014 --f1 0.2 --logD 2.0 --convective_penetration --const The command line prompts for setting the mixing profiles are: Convective boundary layer mixing -------------------------------- Convective penetration: --convective_penetration Exponential diffusive overshoot: --exponential Associated parameter to vary: --f1 input_value Envelope mixing --------------- Constant: --const Internal gravity waves: --IGW_rho1 Vertical shear: --shear Meridional circulation including vertical shear: --shear_meridional Associated parameter to vary: --logD input_value ============================================================ GYRE setup ============================================================ The GYRE_setup/gyre_ad.in file provides the adopted GYRE inlist. The insist parameters that to be modified are: file Omega_rot m freq_min freq_max summary_file The appropriate freq_min and freq_max values to use depends on the input model and choice of Omega_rot.