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A systematic survey for distant galaxy clustersA photographic survey for faint clusters of galaxies has been carried out with fine-grained photographic emulsions using the 1.2 m Schmidt and 5 m Hale telescopes, as well as the 4 m Mayall telescope. A total of 418 clusters have been found with redshifts mostly in the range from 0.15 to 0.92. The survey was planned to minimize distance-dependent selection effects in the resulting catalog. In areas of sky where the deepest search was made, the sample is complete to about z = 0.50; there are 11 clusters per square degree at this limit. At a redshift of 1.0 there should be 63 or 45 clusters per square degree depending on whether q0 is 0.0 or 0.5, provided there is no evolution.
Document ID
19860061792
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Gunn, J. E.
(Princeton University Observatory, NJ; Palomar Observatory, Pasadena, CA, United States)
Hoessel, J. G.
(Space Telescope Science Institute Baltimore, MD, United States)
Oke, J. B.
(Palomar Observatory Pasadena, CA, United States)
Date Acquired
August 12, 2013
Publication Date
July 1, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 306
ISSN: 0004-637X
Subject Category
Astronomy
Accession Number
86A46530
Funding Number(s)
CONTRACT_GRANT: NAS5-25451
CONTRACT_GRANT: NSF AST-82-16717
CONTRACT_GRANT: NSF AST-80-06188
CONTRACT_GRANT: NSF AST-84-20352
CONTRACT_GRANT: NSF AST-76-22111
CONTRACT_GRANT: NSF AST-78-24842
Distribution Limits
Public
Copyright
Other

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