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Galaxy Merger Candidates in High-redshift Cluster Environments

Journal Article · · Astrophysical Journal
;  [1];  [2]; ; ;  [3];  [4];  [5];  [6];  [7];  [8];  [9];  [10]; ; ;  [11]
  1. Department of Physics, McGill University, 3600 Rue University, Montreal, QC, H3A 2T8 (Canada)
  2. Departamento de Ciencias Físicas, Universidad Andres Bello, Fernandez Concha 700, Las Condes 7591538, Santiago, Regin Metropolitana (Chile)
  3. Department of Physics and Astronomy, University of California, Riverside, 900 University Avenue, Riverside, CA 92521 (United States)
  4. Department of Physics and Astronomy, York University, 4700 Keele Street, Toronto, Ontario, Canada, MJ3 1P3 (Canada)
  5. Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON, M5S 3H4 (Canada)
  6. Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States)
  7. Departamento de Astronomía, Universidad de Concepcíon, Casilla 160-C, Concepcíon, Regin del Biobo (Chile)
  8. Argelander-Institute fur Astronomie, Auf dem Hugel 71, D-53121 Bonn (Germany)
  9. Center for Cosmology, Department of Physics and Astronomy, University of California, Irvine, 4129 Frederick Reines Hall, Irvine, CA 92697 (United States)
  10. Australian Astronomical Observatory, P.O. Box 2915, North Ryde NSW 1670 (Australia)
  11. Physics Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States)

We compile a sample of spectroscopically and photometrically selected cluster galaxies from four high-redshift galaxy clusters (1.59

OSTI ID:
22876038
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 843; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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