MESA Inlists for: Black Hole UCXBs as Galactic Low-frequency Gravitational Wave Sources: the He Star Channel

We use the MESA to perform a detailed stellar evolution model for the formation and evolution of BH UCXBs evolving from the He star channel to diagnose their detectability as low-frequency GW sources. In the MESA code, you use the inlist1, inlist_project, and runbinary_extras.f can reproduce our results.