223 citations · 3.3k across the 107 of their papers we have counts for
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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…
Cluster Structure in Cosmological Simulations I: Correlation to Observables, Mass Estimates, and Evolution
Tesla E. Jeltema, Eric J. Hallman, Jack O. Burns +1
We use Enzo, a hybrid Eulerian AMR/N-body code including non-gravitational heating and cooling, to explore the morphology of the X-ray gas in clusters of galaxies and its evolution…
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…
Radio Wavelength Observatories within the Exploration Architecture
J. Lazio, R. J. Macdowall, J. Burns +3
Observations at radio wavelengths address key problems in astrophysics, astrobiology, and lunar structure including the first light in the Universe (the Epoch of Reionization), the…