stellar-astrophysics
The Virtual Planet Simulator
Compact object inspirals with BPASS
MADYS: isochronal parameter determination for young stellar and substellar objects
Rosseland mean opacity at any hydrogen and metal mass fraction, 5 K to 12.6 million K. OPAL joined to Semenov or Ferguson dust, as a callable or a table.
Multi-grid Epic Interpolator for stellar limb DarkEning Models
Tools for asteroseismology of sdB stars using MESA and GYRE models.
