activity
20022009
most citedCosmological Shocks in Adaptive Mesh Refinement Simulations and the Acceleration of Cosmic Rays

161 citations · 407 across the 6 of their papers we have counts for

collaborators

12 papers

astro-ph.CO200936 cited

X-ray Point Sources and Radio Galaxies in Clusters of Galaxies

Quyen N. Hart, John T. Stocke, Eric J. Hallman

Using Chandra imaging spectroscopy and VLA L-band maps, we have identified radio galaxies at P(1.4 GHz) >= 3x10^{23} W Hz^{-1} and X-ray point sources (XPSs) at L(0.3-8 keV) >= 10^…

astro-ph.CO20092 cited

Clusters and Large-Scale Structure: the Synchrotron Keys

L. Rudnick, P. Alexander, H. Andernach +25

For over four decades, synchrotron-radiating sources have played a series of pathfinding roles in the study of galaxy clusters and large scale structure. Such sources are uniquely…

astro-ph2008161 cited

Cosmological Shocks in Adaptive Mesh Refinement Simulations and the Acceleration of Cosmic Rays

Samuel W. Skillman, Brian W. O'Shea, Eric J. Hallman +2

We present new results characterizing cosmological shocks within adaptive mesh refinement N-Body/hydrodynamic simulations that are used to predict non-thermal components of large-s…

astro-ph2007137 cited

Why Do Only Some Galaxy Clusters Have Cool Cores?

Jack O. Burns, Eric J. Hallman, Brennan Gantner +2

Flux-limited X-ray samples indicate that about half of rich galaxy clusters have cool cores. Why do only some clusters have cool cores while others do not? In this paper, cosmologi…

astro-ph200771 cited

The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys

Eric J. Hallman, Brian W. O'Shea, Jack O. Burns +3

We present the first results from a new generation of simulated large sky coverage (~100 square degrees) Sunyaev-Zeldovich effect (SZE) cluster surveys using the cosmological adapt…

astro-ph2005

Ruling the Universe: An Improved Method for Measuring H_0 with Galaxy Clusters

Eric J. Hallman, Jack O. Burns, Patrick M. Motl +1

Withdrawn at the current time due to errors.