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Date and Time of the Query: 2018-12-11 T03:20:18 PST
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For refcode 2002ApJS..142..153S:
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2002ApJS..142..153S Optical and Near-Infrared Photometry of Distant Galaxy Clusters S. A. Stanford Physics Department, University of California, Davis, CA 95616; adam@igpp.ucllnl.org Peter R. Eisenhardt Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109; prme@kromos.jpl.nasa.gov Mark Dickinson Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218; med@stsci.edu B. P. Holden Physics Department, University of California, Davis, CA 95616; bholden@igpp.ucllnl.org and Roberto De Propris Research School of Astronomy and Astrophysics, Australian National University, Weston, ACT 2611, Australia; propris@mso.anu.edu.au Received 2002 February 21; accepted 2002 April 1 ABSTRACT We present optical and near-infrared photometry of 45 clusters of galaxies at 0.1 < z < 1.3. Galaxy catalogs in each cluster were defined at the longest wavelength available, generally the K band, down to approximately 2 mag below M*. We include finding chart images of the band used for catalog definition. The photometry has been used in previously published papers to examine the origin and evolution of galaxies in distant clusters. Subject headings: galaxies: clusters: general - galaxies: evolution - galaxies: formation - galaxies: high-redshift - galaxies: photometry
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