activity
20092024
most citedFIRE-2 Simulations: Physics versus Numerics in Galaxy Formation

1.1k citations · 4.1k across the 76 of their papers we have counts for

collaborators

76 papers

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.GA2023★ 3 cited

The Debris of the "Last Major Merger" is Dynamically Young

Thomas Donlon, Heidi Jo Newberg, Robyn Sanderson +4

The Milky Way's (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the "last major merger." Hypotheses for the origin of t…

astro-ph.GA2023★ 1 cited

Testing the near-far connection with FIRE simulations: inferring the stellar mass function of the proto-Local Group at z > 6 using the fossil record of present-day galaxies

Pratik J. Gandhi, Andrew Wetzel, Michael Boylan-Kolchin +6

The shape of the low-mass (faint) end of the galaxy stellar mass function (SMF) or ultraviolet luminosity function (UVLF) at z > 6 is an open question for understanding which galax…

astro-ph.GA2023★ 7 cited

Bar formation and destruction in the FIRE-2 simulations

Sioree Ansar, Sarah Pearson, Robyn E. Sanderson +5

The physical mechanisms responsible for bar formation and destruction in galaxies remain a subject of debate. While we have gained valuable insight into how bars form and evolve fr…

astro-ph.GA2023★ 11 cited

LMC-driven anisotropic boosts in stream--subhalo interactions

Arpit Arora, Nicolás Garavito-Camargo, Robyn E. Sanderson +4

Dark Matter (DM) subhalos are predicted to perturb stellar streams; stream morphologies and dynamics can constrain the mass distribution of subhalos. Using FIRE-2 simulations of Mi…

astro-ph.GA2023★ 2 cited

Modeling the orbital histories of satellites of Milky Way-mass galaxies: testing static host potentials against cosmological simulations

Isaiah B. Santistevan, Andrew Wetzel, Erik Tollerud +3

Understanding the evolution of satellite galaxies of the Milky Way (MW) and M31 requires modeling their orbital histories across cosmic time. Many works that model satellite orbits…