The MESA and GYRE inlists for Ensemble Asteroseismology for 138 Kepler Metal-poor Red Giants: Stellar Fundamental parameters

This zenodo repo contains the MESA and GYRE inlists in the paper "Ensemble Asteroseismology for 138 Kepler Metal-poor Red Giants: Stellar Fundamental parameters". This repo contains two files both are txt files. inlist_run is the MESA inslit used to compute therotical evolutionary tracks and structural models. gyre.in is the GYRE inlist used to compute theoretical oscillation mode frequency and mode inertia with the structural models computed with MESA. The two inslits can be used with Modules for Experiments in Stellar Astrophysics (MESA), version 12115. For different MESA versions, some parameters in the ientnlist may need modifications. Note that the GYRE tool is now a module of MESA. Both inlists are used for making theoretical predictions in a paper entitled "Ensemble Asteroseismology for 138 Kepler Metal-poor Red Giants: Stellar Fundamental parameters" by Tanda Li et al. accepted by the ApJ. Relavent infomation will be updated after the pulblication.