activity
20162019
most citedELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias

75 citations · 85 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.GA201910 cited

The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations

Shuiyao Huang, Neal Katz, Romeel Davé +5

Many phenomenologically successful cosmological galaxy formation simulations employ kinetic winds to model galactic outflows, a crucial ingredient in obtaining predictions that agr…

astro-ph.GA2018

The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics

Shuiyao Huang, Neal Katz, Romeel Davé +8

We test and improve the numerical schemes in our smoothed particle hydrodynamics (SPH) code for cosmological simulations, including the pressure-entropy formulation (PESPH), a time…

astro-ph.GA201775 cited

ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias

Huiyuan Wang, H. J. Mo, Sihan Chen +17

We examine the quenched fraction of central and satellite galaxies as a function of galaxy stellar mass, halo mass, and the matter density of their large scale environment. Matter…

astro-ph.CO2016

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.GA2016

nIFTy Galaxy Cluster simulations IV: Quantifying the Influence of Baryons on Halo Properties

Weiguang Cui, Chris Power, Alexander Knebe +21

Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and contrast the impact of baryonic physics with a single massive galaxy cluster, run w…