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An IR-selected galaxy cluster at z=1.27

Journal Article · · Astronomical Journal
DOI:https://doi.org/10.1086/118643· OSTI ID:552814
 [1];  [2];  [3]; ;  [4];  [5]
  1. Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
  2. Department of Astronomy, University of Florida, Gainesville, Florida 32611 (United States)
  3. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 (United States)
  4. Department of Astronomy, University of California, Berkeley, California 94720 (United States)
  5. National Optical Astronomy Observatories, Tucson, Arizona 85726 (United States)

We report the discovery of a galaxy cluster at z=1.27. ClG J0848+4453 was found in a near{endash}IR field survey as a high density region of objects with very red J{minus}K colors. Optical spectroscopy of a limited number of 24{approx_lt}R{approx_lt}25 objects in the area shows that 6 galaxies within a 90 arcsec (0.49h{sub 100}{sup {minus}1} Mpc, q{sub 0}=0.1) diameter region lie at z=1.273{plus_minus}0.002. Most of these 6 member galaxies have broad-band colors consistent with the expected spectral energy distribution of a passively-evolving elliptical galaxy formed at high redshift. An additional 2 galaxies located {approximately}2 arcmin from the cluster center are also at z=1.27. Using all 8 of these spectroscopic members, we estimate the velocity dispersion {sigma}=700{plus_minus}180 km s{sup {minus}1}, which is similar to that of Abell richness class R=1 clusters in the present epoch. A deep {ital ROSAT}/PSPC observation detects X-ray emission at the 4.5{sigma} level coincident with the nominal cluster center. Assuming that the X-ray flux is emitted by hot gas trapped in the potential well of a collapsed system (no AGN are known to exist in the area), the resulting X-ray luminosity in the rest frame 0.1{endash}2.4 keV band of L{sub x}=1.5{times}10{sup 44} ergs s{sup {minus}1} suggests the presence of a moderately massive system. ClG J0848+4453 is the highest redshift cluster found in a field survey. {copyright} {ital 1997 American Astronomical Society.}

Research Organization:
Lawrence Livermore National Laboratory
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
552814
Journal Information:
Astronomical Journal, Journal Name: Astronomical Journal Journal Issue: 6 Vol. 114; ISSN ANJOAA; ISSN 0004-6256
Country of Publication:
United States
Language:
English

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