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Title: XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster Cl J120958.9+495352 ( z = 0.902)

Here, observations of relaxed, massive, and distant clusters can provide important tests of standard cosmological models, for example by using the gas mass fraction. To perform this test, the dynamical state of the cluster and its gas properties have to be investigated. X-ray analyses provide one of the best opportunities to access this information and to determine important properties such as temperature profiles, gas mass, and the total X-ray hydrostatic mass. For the last of these, weak gravitational lensing analyses are complementary independent probes that are essential in order to test whether X-ray masses could be biased.
Authors:
 [1] ;  [1] ;  [1] ;  [2] ;  [3] ;  [4] ;  [5] ;  [1] ;  [6]
  1. Univ. Bonn, Bonn (Germany)
  2. Harvard Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  3. Stanford Univ., Stanford, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
  4. Leiden Univ., Leiden (The Netherlands)
  5. Univ. of Chicago, Chicago, IL (United States)
  6. Cadmus, Madison, WI (United States)
Publication Date:
Grant/Contract Number:
AC02-76SF00515
Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 610; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Research Org:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Org:
USDOE
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; galaxies: clusters: general; galaxies: clusters: individual: Cl J120958.9+495352; X-rays: galaxies: clusters; gravitational lensing: weak
OSTI Identifier:
1437242

Tholken, Sophia, Schrabback, Tim, Reiprich, Thomas H., Lovisari, Lorenzo, Allen, Steven W., Hoekstra, Henk, Applegate, Douglas, Buddendiek, Axel, and Hicks, Amalia. XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster Cl J120958.9+495352 (z = 0.902). United States: N. p., Web. doi:10.1051/0004-6361/201730913.
Tholken, Sophia, Schrabback, Tim, Reiprich, Thomas H., Lovisari, Lorenzo, Allen, Steven W., Hoekstra, Henk, Applegate, Douglas, Buddendiek, Axel, & Hicks, Amalia. XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster Cl J120958.9+495352 (z = 0.902). United States. doi:10.1051/0004-6361/201730913.
Tholken, Sophia, Schrabback, Tim, Reiprich, Thomas H., Lovisari, Lorenzo, Allen, Steven W., Hoekstra, Henk, Applegate, Douglas, Buddendiek, Axel, and Hicks, Amalia. 2018. "XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster Cl J120958.9+495352 (z = 0.902)". United States. doi:10.1051/0004-6361/201730913.
@article{osti_1437242,
title = {XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster Cl J120958.9+495352 (z = 0.902)},
author = {Tholken, Sophia and Schrabback, Tim and Reiprich, Thomas H. and Lovisari, Lorenzo and Allen, Steven W. and Hoekstra, Henk and Applegate, Douglas and Buddendiek, Axel and Hicks, Amalia},
abstractNote = {Here, observations of relaxed, massive, and distant clusters can provide important tests of standard cosmological models, for example by using the gas mass fraction. To perform this test, the dynamical state of the cluster and its gas properties have to be investigated. X-ray analyses provide one of the best opportunities to access this information and to determine important properties such as temperature profiles, gas mass, and the total X-ray hydrostatic mass. For the last of these, weak gravitational lensing analyses are complementary independent probes that are essential in order to test whether X-ray masses could be biased.},
doi = {10.1051/0004-6361/201730913},
journal = {Astronomy and Astrophysics},
number = ,
volume = 610,
place = {United States},
year = {2018},
month = {3}
}