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20112020
most citedMUFASA: Galaxy Formation Simulations With Meshless Hydrodynamics

337 citations · 2k across the 21 of their papers we have counts for

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Showing astro-ph.COShow all

8 papers · 1 filter

astro-ph.CO2016★ 50 cited

The Soft, Fluctuating UVB at as Traced by C IV, SiIV, and CII

K. Finlator, B. D. Oppenheimer, R. Davé +3

The sources that drove cosmological reionization left clues regarding their identity in the slope and inhomogeneity of the ultraviolet ionizing background (UVB): Bright quasars (QS…

astro-ph.CO2014★ 34 cited

The rise and fall of a challenger: the Bullet Cluster in Cold Dark Matter simulations

Robert Thompson, Romeel Davé, Kentaro Nagamine

The Bullet Cluster has provided some of the best evidence for the cold dark matter () model via direct empirical proof of the existence of collisionless dark matter,…

astro-ph.CO2013★ 173 cited

Tracing Inflows and Outflows with Absorption Lines in Circumgalactic Gas

Amanda Brady Ford, Romeel Davé, Benjamin D. Oppenheimer +4

We examine how HI and metal absorption lines within low-redshift galaxy halos trace the dynamical state of circumgalactic gas, using cosmological hydrodynamic simulations that incl…

astro-ph.CO2013★ 25 cited

Dust properties of Lyman break galaxies in cosmological simulations

Hidenobu Yajima, Kentaro Nagamine, Robert Thompson +1

Recent observations have indicated the existence of dust in high-redshift galaxies, however, the dust properties in them are still unknown. Here we present theoretical constraints…

astro-ph.CO2013★ 56 cited

Impact of H_2-based star formation model on the z>=6 luminosity function and the ionizing photon budget for reionization

Jason Jaacks, Robert Thompson, Kentaro Nagamine

We present the results of a numerical study examining the effect of H_2-based star formation (SF) model on the rest-frame UV luminosity function and star formation rate function (S…

astro-ph.CO2013★ 44 cited

Molecular hydrogen regulated star formation in cosmological SPH simulations

Robert Thompson, Kentaro Nagamine, Jason Jaacks +1

It has been shown observationally that star formation (SF) correlates tightly with the presence of molecular hydrogen (H). Therefore it would be important to investigate its im…