NASA has selected Fiona McCluskey for a Future Investigators in NASA Earth and Space Science and Technology (FINESST) award! This grant will fund the final 2 years of Fiona’s PhD project: Deciphering Galactic Disk Formation: Galactic Archaeology in a Cosmological Context. Congratulations Fiona!
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!
Dr. Isaiah Santistevan
Dr. lsaiah Santistevan is our group’s second graduating PhD student! He completed his PhD dissertation on Modelling the Formation and Evolution of Satellite Galaxies in Cosmological Simulations. He will start as a postdoc at Lawrence Livermore National Laboratory. Congratulations Dr. Santistevan!
Pratik Gandhi awarded Frontera Fellowship
The Texas Advanced Computing Center (TACC)Â 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!
Dr. Jenna Samuel
Dr. Jenna Samuel is our group’s first graduating PhD student! She completed her PhD dissertation on Local Group Satellite Galaxies in Cosmological Simulations. She will start as an NSF Astronomy & Astrophysics Postdoctoral Fellow in the Department of Astronomy at the University of Texas, Austin. Congratulations Dr. Samuel!
Isaiah Santistevan awarded NASA FINESST
NASA selected Isaiah Santistevan for a Future Investigators in NASA Earth and Space Science and Technology (FINESST) award! This grant will fund the final 2 years of Isaiah’s PhD project: Modeling the Cosmological Evolution of Satellite Dwarf Galaxies in 6D Phase Space. Congratulations Isaiah!
UC Davis article: Milky Way galaxy merger
UC Davis College of Letters & Science highlighted our recent research in their article: Simulations Reveal Signs of Galaxy Mergers in Milky Way Disk. PhD student Isaiah Santistevan led this research, to understand how a merger with another galaxy likely shaped the orbits of the most ancient and metal-poor stars in our Milky Way galaxy today.
Sky & Telescope article: plane of satellites
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, 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
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!