Research Projects
My research focuses on using photometric surveys to characterize resolved stars and their line-of-sight extinction in nearby galaxies like the Magellanic Clouds and M31. Through multi-phase tracers like dust extinction, I study the structure of the interstellar medium (ISM). I am primarily interested in understanding how the multi-scale structure of the ISM changes as a function of metallicity and galactic environment, and how these changes influence star formation and the impact of stellar feedback.
I am involved in several photometric surveys of nearby galaxies. Some of my recent work and ongoing projects from these collaborations are described below.
