I am a postdoctoral researcher at Michigan State University in the department of Physics and Astronomy.
I work with Professor Wolfgang Kerzendorf and the
Kerzendorf Group modeling stars and searching for
surviving companions of type Ia supernovae to learn about their progenitor systems and test
different progenitor theories. I use statistical methods capitalizing on the revolutionary new GAIA
mission as well as archival Hubble data to investigate the stellar populations in supernova
remnants. I work at the intersection of observation and theory, making detailed models of stellar
atmospheres to simulate escaping stellar light and then fitting those models to observations to
learn about the structure and composition of stars.
I am the primarily developer on the open-source STARDIS
code, which solves the radiative transfer equation in the outer layers of a star to simulate
light passing through it.