activity
20162026
most citedFIRE-3: Updated Stellar Evolution Models, Yields, & Microphysics and Fitting Functions for Applications in Galaxy Simulations

139 citations · 1.1k across the 69 of their papers we have counts for

collaborators
Showing 2024Show all

9 papers · 1 filter

astro-ph.GA2024★ 3 cited

Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies

Nora Shipp, Alexander H. Riley, Christine M. Simpson +7

Galaxies like the Milky Way are surrounded by complex populations of satellites at all stages of tidal disruption. In this paper, we present a dynamical study of the disrupting sat…

astro-ph.GA2024★ 1 cited

StreamGen: Connecting Populations of Streams and Shells to Their Host Galaxies

Adriana Dropulic, Nora Shipp, Stacy Kim +3

In this work, we study how the abundance and dynamics of populations of disrupting satellite galaxies change systematically as a function of host galaxy properties. We apply a theo…

astro-ph.GA2024★ 2 cited

How DREAMS are made: Emulating Satellite Galaxy and Subhalo Populations with Diffusion Models and Point Clouds

Tri Nguyen, Francisco Villaescusa-Navarro, Siddharth Mishra-Sharma +16

The connection between galaxies and their host dark matter (DM) halos is critical to our understanding of cosmology, galaxy formation, and DM physics. To maximize the return of upc…

astro-ph.GA2024★ 6 cited

Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?

Dylan Folsom, Mariangela Lisanti, Lina Necib +3

Observations of the Milky Way's stellar halo find that it is predominantly comprised of a radially biased population of stars, dubbed the Gaia Sausage--Enceladus, or GSE. These sta…

astro-ph.GA2024★ 5 cited

The imprint of dark matter on the Galactic acceleration field

Arpit Arora, Robyn E. Sanderson, Sukanya Chakrabarti +6

Measurements of the accelerations of stars enabled by time-series extreme-precision spectroscopic observations, from pulsar timing, and from eclipsing binary stars in the Solar Nei…

astro-ph.GA2024★ 2 cited

Introducing the DREAMS Project: DaRk mattEr and Astrophysics with Machine learning and Simulations

Jonah C. Rose, Paul Torrey, Francisco Villaescusa-Navarro +27

We introduce the DREAMS project, an innovative approach to understanding the astrophysical implications of alternative dark matter models and their effects on galaxy formation and…

astro-ph.GA2024★ 8 cited

Confronting the Diversity Problem: The Limits of Galaxy Rotation Curves as a tool to Understand Dark Matter Profiles

Isabel S. Sands, Philip F. Hopkins, Xuejian Shen +9

While galaxy rotation curves provide one of the most powerful methods for measuring dark matter profiles in the inner regions of rotation-supported galaxies, at the dwarf scale the…

astro-ph.GA2024

Signatures of tidal disruption of the Hercules ultra-faint dwarf galaxy

Xiaowei Ou, Anirudh Chiti, Nora Shipp +6

The Hercules ultra-faint dwarf galaxy (UFD) has long been hypothesized to be tidally disrupting, yet no conclusive evidence has been found for tidal disruption owing partly to diff…

astro-ph.GA2024★ 15 cited

The Escape Velocity Profile of the Milky Way from Gaia DR3

Cian Roche, Lina Necib, Tongyan Lin +2

The escape velocity profile of the Milky Way offers a crucial and independent measurement of its underlying mass distribution and dark matter properties. Using a sample of stars fr…