Testing for X-Ray-SZ Differences and Redshift Evolution in the X-Ray Morphology of Galaxy Clusters

Testing for X-Ray-SZ Differences and Redshift Evolution in the X-Ray Morphology of Galaxy Clusters

We present a quantitative study of the X-ray morphology of galaxy clusters, as a function of their detection method and redshift. We analyze two separate samples of galaxy clusters: a sample of 36 clusters at 0.35 < z < 0.9 selected in the X-ray with the ROSAT PSPC 400 deg 2 survey, and a samp...

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Main Authors: Nurgaliev, D. (Author), Benson, B. A. (Author), Bleem, L. (Author), Bocquet, S. (Author), Forman, W. R. (Author), Garmire, G. P. (Author), Gupta, N. (Author), Hlavacek-Larrondo, J. (Author), Mohr, J. J. (Author), Nagai, D. (Author), Rapetti, D. (Author), Stark, A. A. (Author), Stubbs, C. W. (Author), Vikhlinin, A. (Author), McDonald, Michael A. (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-11-01T15:48:43Z.
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