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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 thr…
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…
SPT-CL J0417-4748: A Deep Chandra Study of a Relaxed Galaxy Cluster Without Central Star Formation
Taweewat Somboonpanyakul, Adam B. Mantz, Steven W. Allen +7
We present an in-depth Chandra X-ray analysis of the galaxy cluster SPT-CL J04174748 (hereafter SPT J0417), at z = 0.58, with a focus on its thermodynamic properties and the app…
Multiwavelength Characterization of a Dynamically Relaxed Cool Core Galaxy Cluster at
Anthony M. Flores, Adam B. Mantz, Steven W. Allen +5
We present imaging and spectroscopic analyses of Chandra and XMM-Newton observations of ACT-CL J0123.50428, one of the most massive, highest redshift galaxy clusters detected wi…
Deep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-3537
Haley R. Stueber, Adam B. Mantz, Steven W. Allen +10
Galaxy clusters serve as a unique and valuable laboratory for probing cosmological models and understanding astrophysics at the high-mass limit of structure formation. Clusters tha…
A Generative Model for Realistic Galaxy Cluster X-ray Morphologies
Maya Benyas, Jordan Pfeifer, Adam B. Mantz +2
The X-ray morphologies of clusters of galaxies display significant variations, reflecting their dynamical histories and the nonlinear dependence of X-ray emissivity on the density…