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20122025
most citedFIRE-2 Simulations: Physics versus Numerics in Galaxy Formation

1.1k citations · 8.5k across the 56 of their papers we have counts for

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Showing 2013Show all

5 papers · 1 filter

astro-ph.CO2013★ 238 cited

Sterile neutrino dark matter bounds from galaxies of the Local Group

Shunsaku Horiuchi, Philip J. Humphrey, Jose Onorbe +3

We show that the canonical oscillation-based (non-resonant) production of sterile neutrino dark matter is inconsistent at % confidence with observations of galaxies in the Loc…

astro-ph.CO2013★ 333 cited

ELVIS: Exploring the Local Volume in Simulations

Shea Garrison-Kimmel, Michael Boylan-Kolchin, James Bullock +1

We introduce a set of high-resolution dissipationless simulations that model the Local Group (LG) in a cosmological context: Exploring the Local Volume in Simulations (ELVIS). The…

astro-ph.GA2013★ 41 cited

On the stark difference in satellite distributions around the Milky Way and Andromeda

Basilio Yniguez, Shea Garrison-Kimmel, Michael Boylan-Kolchin +1

We compare spherically-averaged radial number counts of bright (> 10^5 Lsun) dwarf satellite galaxies within 400 kpc of the Milky Way (MW) and M31 and find that the MW satellites a…

astro-ph.CO2013★ 143 cited

How to Zoom: Bias, Contamination, and Lagrange Volumes in Multimass Cosmological Simulations

Jose Oñorbe, Shea Garrison-Kimmel, Ariyeh H. Maller +3

We perform a suite of multimass cosmological zoom simulations of individual dark matter halos and explore how to best select Lagrangian regions for resimulation without contaminati…

astro-ph.CO2013★ 186 cited

Can Feedback Solve the Too Big to Fail Problem?

Shea Garrison-Kimmel, Miguel Rocha, Michael Boylan-Kolchin +2

The observed central densities of Milky Way dwarf spheroidal galaxies (dSphs) are significantly lower than the densities of the largest (Vmax about 35 km/s) subhalos found in dissi…