Asteroseismology with MESA

In this series of labs, we will familiarise ourselves with applying GYRE — a tool for computing the normal-mode frequencies of spherical stars — to stellar models produced with MESA. This series of labs is mainly intended to teach you how to do asteroseismology using MESA — rather than asteroseismology itself — but we have also prepared a brief primer on asteroseismology proper here.

Slides for the Friday labs can be found here.