4 papers
Clusters Hiding Under Millimeter Sources (CHUMS) I: Extreme CHUMS
Harshda Saxena, Adam B. Mantz, Jack Sayers +2
Galaxy cluster abundance provides a powerful probe of the CDM model and enables precise constraints on cosmological parameters. Millimeter-wavelength surveys detect clusters th…
Ruminations Upon the Modeling of X-ray Foregrounds, Backgrounds and Faint Sources
Adam B. Mantz, Anthony M. Flores, Taweewat Somboonpanyakul +4
With the goal of extracting as much information as possible from Chandra and XMM-Newton observations of faint, diffuse sources such as galaxy clusters, as well as those of future X…
The Cluster Evolutionary Reference Ensemble at Low- (CEREAL) Sample of Galaxy Clusters I: X-ray Morphological Properties and Demographics
Laurel White, Michael McDonald, Steven W. Allen +8
With rapid improvements in the assembly of large samples of galaxy clusters, we are approaching the ability to study clusters at . Evolutionary studies comparing these d…
AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03
A. Mhatre, M. C. Powell, S. Yuan +10
The large-scale environments of active galactic nuclei (AGN) reveal important information on the growth and evolution of supermassive black holes (SMBHs). Previous AGN clustering m…