activity
19952013
most citedHalo Formation in Warm Dark Matter Models

1.1k citations · 4.3k across the 40 of their papers we have counts for

collaborators

40 papers

astro-ph.CO2013★ 79 cited

The Stellar Mass Growth of Brightest Cluster Galaxies in the IRAC Shallow Cluster Survey

Yen-Ting Lin, Mark Brodwin, Anthony H. Gonzalez +4

The details of the stellar mass assembly of brightest cluster galaxies (BCGs) remain an unresolved problem in galaxy formation. We have developed a novel approach that allows us to…

astro-ph.CO2012★ 9 cited

Calibration of Nonthermal Pressure in Global Dark Matter Simulations of Clusters of Galaxies

Paul Bode, Jeremiah P. Ostriker, Renyue Cen +1

We present a new method for incorporating nonthermal pressure from bulk motions of gas into an analytic model of the intracluster medium in clusters of galaxies, which is based on…

astro-ph.CO2010★ 12 cited

Where are the missing baryons in clusters?

Bilhuda Rasheed, Neta Bahcall, Paul Bode

Observations of clusters of galaxies suggest that they contain significantly fewer baryons (gas plus stars) than the cosmic baryon fraction. This `missing baryon' puzzle is especia…

astro-ph.CO2010★ 108 cited

Templates for the Sunyaev-Zel'dovich Angular Power Spectrum

Hy Trac, Paul Bode, Jeremiah P. Ostriker

We present templates for the Sunyaev-Zel'dovich (SZ) angular power spectrum based on four models for the nonlinear gas distribution. The frequency-dependent SZ temperature fluctuat…

astro-ph.CO2009★ 210 cited

Simulations of the Microwave Sky

Neelima Sehgal, Paul Bode, Sudeep Das +5

We create realistic, full-sky, half-arcminute resolution simulations of the microwave sky matched to the most recent astrophysical observations. The primary purpose of these simula…

astro-ph.CO2009★ 93 cited

Exploring the Energetics of Intracluster Gas with a Simple and Accurate Model

Paul Bode, Jeremiah P. Ostriker, Alexey Vikhlinin

The state of the hot gas in clusters of galaxies is investigated with a set of model clusters, created by assuming a polytropic equation of state (Gamma=1.2) and hydrostatic equili…