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Title: THE MASSIVE AND DISTANT CLUSTERS OF WISE SURVEY: MOO J1142+1527, A 10{sup 15}M{sub ⊙} GALAXY CLUSTER AT z = 1.19

Journal Article · · Astrophysical Journal Letters
;  [1]; ;  [2]; ;  [3]; ;  [4];  [5];  [6]; ; ; ;  [7]; ; ;  [8];  [9];  [10];  [11] more »; « less
  1. Department of Astronomy, University of Florida, Gainesville, FL 32611-2055 (United States)
  2. Department of Physics and Astronomy, University of Missouri, 5110 Rockhill Road, Kansas City, MO 64110 (United States)
  3. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)
  4. Steward Observatory, University of Arizona, Tucson, AZ 85121 (United States)
  5. Department of Physics, University of California, One Shields Avenue, Davis, CA 95616 (United States)
  6. Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States)
  7. Physics Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States)
  8. Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 (United States)
  9. Institute of Astronomy and Astrophysics, Academica Sinica, Taipei, Taiwan (China)
  10. Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305 (United States)
  11. California Institute of Technology, Owens Valley Radio Observatory, Big Pine, CA 93513 (United States)

We present confirmation of the cluster MOO J1142+1527, a massive galaxy cluster discovered as part of the Massive and Distant Clusters of WISE Survey. The cluster is confirmed to lie at z = 1.19, and using the Combined Array for Research in Millimeter-wave Astronomy we robustly detect the Sunyaev–Zel’dovich (SZ) decrement at 13.2σ. The SZ data imply a mass of M{sub 200m} = (1.1 ± 0.2) × 10{sup 15}M{sub ⊙}, making MOO J1142+1527 the most massive galaxy cluster known at z > 1.15 and the second most massive cluster known at z > 1. For a standard ΛCDM cosmology it is further expected to be one of the ∼5 most massive clusters expected to exist at z ≥ 1.19 over the entire sky. Our ongoing Spitzer program targeting ∼1750 additional candidate clusters will identify comparably rich galaxy clusters over the full extragalactic sky.

OSTI ID:
22518748
Journal Information:
Astrophysical Journal Letters, Vol. 812, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 2041-8205
Country of Publication:
United States
Language:
English