Supporting information for v1 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 `7619a75` in this GitHub repo: https://github.com/adamjermyn/conv_trends The metallicities are as follows: main_Z_time_2021_12_14_12_59_57_sha_3d07 - Z = 0.002 (SMC) main_Z_time_2021_12_14_13_00_09_sha_5afc - Z = 0.006 (LMC) main_Z_time_2021_12_14_13_00_18_sha_c740 - Z = 0.01 main_Z_time_2021_12_14_13_00_27_sha_db89 - Z = 0.014 (MW)