Asteroseismic Structure Inversions of Main-Sequence Solar-like Oscillators with Convective Cores.

This repository contains the accompanying insists and run_star_extras files for Buchele et al. (2025): Asteroseismic Structure Inversions of Main-Sequence Solar-like Oscillators with Convective Cores. The MESA version used is r22.05.1. We have modified the /star/private/pulse_fgong.f90 file in the MESA source code to output the Gamma1 derivatives that are necessary to compute u-Y kernels by replacing the file with the version from https://github.com/MESAHub/mesa/pull/431. Additionally, we use the MESA SDK versions 22.6.1 and the GYRE version 6.0 that is included with the r22.05.1 release of MESA. The directory grid_base contains the inlist which set the parameters that do not change across the tracks of our grid Inlist_all includes parameters that are constant across all tracks and evolutionary stagesInlist_prems includes parameters for the pre-main sequence evolution of all tracksInlist_ms includes parameters for the main sequence evolution of all tracksrun_star_extras/save_freqs.run_star_extras.f90 includes the code used to save frequencies during the evolutionrun_star_extras/fit_Age.run_star_extras.f90 includes the code which stops the evolution at a given agegyre.in includes parameters for calculating of frequencies using GYRE The directory reference_models provides the inlists to generate our reference model for each star in our sample. This directory also includes the FGONG structure files of the computed reference models. Each file is labeled with the identifier used in the text, typically the KIC number. The mixing_changes directory provides the inlists to generate the models with modified input physics.core_pc: Core Convective Penetrationdiffusion: Diffusion and Gravitational Settlingrad_lev: Diffusion, Settling, Radiative Acceleration