I am an assistant professor in the department of physics at UC Davis. I earned my Ph.D. in astrophysics at UC Berkeley and pursued postdoctoral research at Yale University, Caltech, and Carnegie Observatories. Read more about my research and my background.
I am fortunate to pursue research with the fantastic group below.
Sarah Loebman is a NASA Hubble Fellow and UC Davis Chancellor’s Postdoctoral Fellow. Sarah is a stellar dynamicist at heart who works on all aspects of the Milky Way, from the formation and evolution of stars and star clusters in its disk, including their dynamics and elemental abundances, to its diffuse stellar halo, including how to measure the mass and shape of the Milky Way’s dark-matter halo. Sarah lives at the intersection of theory/simulation and observations, and she also is a leader in Big Data techniques.
Samantha Benincasa is a postdoctoral research scholar. She works on simulations of galaxy formation to understand the inter-stellar medium (ISM) gas in the Milky Way and nearby galaxies. She is particularly interested in giant molecular clouds (GMCs): their lifetimes, dynamics in the disk how they give rise to star formation, and how they are affected by stellar feedback.
Jenna Samuel works on low-mass ‘dwarf’ galaxies, in particular, the satellites of the Milky Way and Andromeda (M31). Jenna’s current research focuses on the origin of their spatial and velocity distributions, including the meaning and origin of observed planes of satellites. She also is interested in understanding (and disentangling) the roles of (internal) stellar feedback and (external) host halo environment on the evolution of dwarf galaxies.
Isaiah Santistevan works on the `near-far connection’: understanding the role of nearby dwarf galaxies during the epoch of reionization, including how we can infer the contribution of low-mass galaxies to the UV luminosity function across cosmic time. Isaiah also is interested in developing new models, using our cosmological simulations, to infer the full orbital histories of all of the dwarf galaxies in the Local Group.
Matt Bellardini works on the formation of the disk of the Milky Way, including stellar and gas dynamics, thin+thick disk formation, and how to use stellar ages and abundances to reconstruct the formation history of the Milky Way via ‘galactic archaeology’.
Sierra Chapman is an undergraduate student majoring in physics. Her research focuses on predictions for the population of dark-matter subhalos in the halo of the Milky Way, including encounter rates of subhalos with the Milky Way’s disk and stellar streams.
Theodore is our group’s Chief Morale Officer. He earned his Pretty hairy Dog (Ph.D.) degree at Caltech in 2015 (advisor: JoAnn Boyd) and also pursued a postdog fellowship at Carnegie Observatories. As you can see above, he basically runs our group.