I recently graduated with my PhD in Astrophysics from Caltech, working with Prof. Phil Hopkins on understanding the role of magnetic fields and cosmic rays in galaxy formation and evolution. I’m particularly interested in leveraging theory, often through the use of high-resolution, cosmological simulations of galaxy formation, to make detailed predictions of a wide swath of observables across the electromagnetic spectrum. My methodology has 1) physically interpreted highly indirect and formalistic observational inferences and 2) constrained highly uncertain non-thermal physics from the smallest scales in the interstellar medium to the largest expanses of intergalactic space. My interest in magnetic fields and cosmic rays and galaxies is broad; ranging from questions of how they can alter the the halos of galaxies to understanding amplification mechanisms of the magnetic fields over cosmological time.

I am proud to have grown up on the island of Jamaica, before moving to the United States in middle school. I then lived in the New York metropole and rural and suburban Iowa, leading to undergraduate degrees in Physics, Astronomy, and Mathematics at the University of Iowa, where I worked with Prof. Phil Kaaret and Prof. Hai Fu on studying metallicity effects on high-mass X-ray binary populations, and understanding cool gas accretion in a high (now with JWST, maybe medium) redshift galaxy. During my undergraduate studies, I had the very fortunate opportunity to spend a semester and a summer in Scotland, where I attended the University of Edinburgh. While there, I worked with Prof. Sadegh Khochfar, Prof. Jose Onorbe, and Prof. Britton Smith on studying Local Group analogs in large volume cosmological simulations.