Dr. Matt Bellardini

Dr. Matt Bellardini

Dr. Matt Bellardini is our group’s third graduating PhD student! He completed his PhD dissertation on Chemical Evolution Across Cosmic Time: Stellar Elemental Abundance Patterns and Radial Redistribution in Cosmological Simulations. Matt is searching for industry jobs in the Seattle area. Congratulations Dr. Bellardini!

Pratik Gandhi awarded Frontera Fellowship

The Texas Advanced Computing Center (TACC) selected Pratik Gandhi for a Frontera Computational Science Fellowship! This fellowship will provide one year of tuition and stipend, including a computing allocation on Frontera and collaboration and mentorship with members of TACC, for Pratik’s PhD project: Near-Far Connection: Using the Stellar Fossil Record of Local Group Dwarf Galaxies to Probe the Epoch of Reionization. Congratulations Pratik!

Sky & Telescope article: plane of satellites

The Alignment of the Milky Way’s Entourage, Explained

Sky & Telescope highlighted our recent research in their article: The Alignment of the Milky Way’s Entourage, Explained. PhD student Jenna Samuel led this work, to understand the origin of the thin plane of satellite galaxies around the Milky Way, including the likely important role that the Large Magellanic Cloud has played in causing this planar structure.

Jenna Samuel awarded NSF Postdoctoral Fellowship

Jenna Samuel

Jenna Samuel, our group’s first graduating PhD student, has been awarded an NSF Astronomy & Astrophysics Postdoctoral Fellowship from the National Science Foundation! Jenna will take this fellowship to the Department of Astronomy at the University of Texas, Austin this fall to pursue her project: Modeling the physics of gas removal and quenching in Local Group satellite galaxies with next-generation simulations. Congratulations Jenna!

first student-led paper from our group: radial distribution of satellite galaxies

Radial distance distribution of satellite galaxies around MW-mass galaxies in the FIRE-2 simulations, as compared with the MW and M31

We are excited to announce the first student-led paper from our group, from PhD student Jenna Samuel: A profile in FIRE: resolving the radial distributions of satellite dwarf galaxies in the Local Group with simulations. Jenna examined the radial distance distribution of satellite galaxies around MW/M31-mass galaxies in our FIRE simulations, which she showed are consistent with the Local Group and with MW-like galaxies from the SAGA survey. Interestingly, more massive host galaxies have fewer satellites at small distances, because of tidal destruction from the host galaxy. Jenna also quantified the destruction of subhalos by comparing our baryonic simulations to their dark matter-only versions, finding 10x fewer subhalos within the inner 20 kpc. Finally, Jenna applied observational completeness within the LG to our simulations, predicting 2-10 more satellites with stellar mass > 1e5 Msun to be discovered around the MW and 6-9 around M31. Congratulations to Jenna for an excellent first paper!