activity
20002022
most citedEffects of Preheating on X-ray Scaling Relations in Galaxy Clusters

181 citations · 418 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2022★ 41 cited

Machine-learning classification of astronomical sources: estimating F1-score in the absence of ground truth

A. Humphrey, W. Kuberski, J. Bialek +5

Machine-learning based classifiers have become indispensable in the field of astrophysics, allowing separation of astronomical sources into various classes, with computational effi…

astro-ph.CO2009★ 6 cited

Hydrodynamic simulations of correlation and scatter in galaxy cluster maps

A. Finoguenov, A. J. R. Sanderson, J. J. Mohr +2

The two dimensional structure of hot gas in galaxy clusters contains information about the hydrodynamical state of the cluster, which can be used to understand the origin of scatte…

astro-ph2005★ 143 cited

Effects of Mergers and Core Structure on the Bulk Properties of Nearby Galaxy Clusters

Timothy B. O'Hara, Joseph J. Mohr, John J. Bialek +1

We use morphological measurements and the scatter of clusters about observed and simulated scaling relations to examine the impact of merging and core-related phenomena on the stru…

astro-ph2002★ 9 cited

Studying Dark Energy with Galaxy Cluster Surveys

Joseph J. Mohr, Brian OShea, August E. Evrard +2

Galaxy cluster surveys provide a powerful means of studying the density and nature of the dark energy. The redshift distribution of detected clusters in a deep, large solid angle S…

astro-ph2002★ 38 cited

A Cold Front in a Preheated Galaxy Cluster

John J. Bialek, August E. Evrard, Joseph J. Mohr

We present a simulated cluster of galaxies, modeled with a pre-heated intracluster medium, that exhibits X-ray features similar to the `cold fronts' seen in Chandra observations. M…

astro-ph2000★ 181 cited

Effects of Preheating on X-ray Scaling Relations in Galaxy Clusters

John J. Bialek, August E. Evrard, Joseph J. Mohr

The failure of purely gravitational models of X-ray cluster formation to reproduce basic observed properties of the local cluster population suggests the need for one or more addit…