Astrophysics

Prior to working as a quant, Sarah worked on several astrophysics publications as a student at UCLA:

The Mass-Radius Relation for Star-Forming Galaxies at z ~ 1.5-3.0

An HST/WFC3-IR Morphological Survey of Galaxies at z = 1.5-3.6: I. Survey Description and Morphological Properties of Star Forming Galaxies

An HST/WFC3-IR Morphological Survey of Galaxies at z = 1.5-3.6: II. The Relation between Morphology and Gas-Phase Kinematics