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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…
The Hierarchical Build-Up of Massive Galaxies and the Intracluster Light since z=1
Charlie Conroy, Risa H. Wechsler, Andrey V. Kravtsov
We use a set of simulation-based models for the dissipationless evolution of galaxies since z=1 to constrain the fate of accreted satellites embedded in dark matter subhalos. These…