Supporting information for v2 of ``A Transparent Window into Early-Type Stellar Variability''

These folders contain grids of main-sequence stellar models computed four different metallicities and masses varying from 0.1-60 MSun. Models were computed using MESA r15140 following commit `964e07d` in this GitHub repo: https://github.com/adamjermyn/conv_trends. Changes from the previous version include: - Fixed a bug in calculating certain averages over the convection zone. - Incorporated the effects of radiation pressure on the Rayleigh number. - Increased time resolution of models. The metallicities are as follows: main_Z_time_2022_01_18_13_56_00_sha_ef8c - Z = 0.002 (SMC) main_Z_time_2022_01_18_13_56_06_sha_adbd - Z = 0.006 (LMC) main_Z_time_2022_01_18_13_56_13_sha_e814 - Z = 0.01<br> main_Z_time_2022_01_18_13_56_19_sha_f7ec - Z = 0.014 (MW)