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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)

Journal Article · · Astronomy and Astrophysics
 [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)
+ Show Author Affiliations

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.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1437242
Journal Information:
Astronomy and Astrophysics, Journal Name: Astronomy and Astrophysics Vol. 610; ISSN 0004-6361
Publisher:
EDP SciencesCopyright Statement
Country of Publication:
United States
Language:
English

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79 ASTRONOMY AND ASTROPHYSICS
X-rays: galaxies: clusters
galaxies: clusters: general
galaxies: clusters: individual: Cl J120958.9+495352
gravitational lensing: weak