229 citations · 885 across the 10 of their papers we have counts for
14 papers · 1 filter
Mapping the Dark Matter From UV Light at High Redshift: An Empirical Approach to Understand Galaxy Statistics
K. -S. Lee, M. Giavalisco, C. Conroy +5
We present a simple formalism to interpret two galaxy statistics, the UV luminosity function and two-point correlation functions for star-forming galaxies at z~4, 5, 6 in the conte…
The Void Phenomenon Explained
Jeremy L. Tinker, Charlie Conroy
We use high-resolution N-body simulations, combined with a halo occupation model of galaxy bias, to investigate voids in the galaxy distribution. Our goal is to address the 'void p…
Thermal Balance in the Intracluster Medium: Is AGN Feedback Necessary?
Charlie Conroy, Jeremiah P. Ostriker
A variety of physical heating mechanisms are combined with radiative cooling to explore, via one dimensional hydrodynamic simulations, the expected thermal properties of the intrac…
The Varied Fates of z~2 Star-forming Galaxies
Charlie Conroy, Alice E. Shapley, Jeremy L. Tinker +2
Star-forming galaxies constitute the majority of galaxies with stellar masses >10^10 M_Sun/h^2 at z~2 and dominate the star-formation rate density of the Universe at this early epo…
Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment?
Jeremy L. Tinker, Charlie Conroy, Peder Norberg +3
We use measurements of the projected galaxy correlation function w_p and galaxy void statistics to test whether the galaxy content of halos of fixed mass is systematically differen…
Constraints on the merging timescale of luminous red galaxies, or, where do all the halos go?
Charlie Conroy, Shirley Ho, Martin White
In the LCDM cosmology dark matter halos grow primarily through the accretion of smaller halos. Much of the mass in a halo of 10^14Msun comes in through accretion of ~10^13Msun halo…