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...

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Bibliographic Details
Main Authors: Nurgaliev, D., Benson, B. A., Bleem, L., Bocquet, S., Forman, W. R., Garmire, G. P., Gupta, N., Hlavacek-Larrondo, J., Mohr, J. J., Nagai, D., Rapetti, D., Stark, A. A., Stubbs, C. W., Vikhlinin, A., McDonald, Michael A.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Published: IOP Publishing 2017
Online Access:http://hdl.handle.net/1721.1/112105
https://orcid.org/0000-0001-5226-8349

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http://hdl.handle.net/1721.1/112105
https://orcid.org/0000-0001-5226-8349

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