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The Hawaii K-band galaxy survey. 1: Deep K-band imagingWe present the results of a very deep K-band survey with a 5 sigma total galaxy magnitude limit of K = 21.9 in the deepest field. A 5 sigma K-band-selected sample of 123 galaxies is presented, together with their optical colors. Only three galaxies in this sample are not detected at the 1 sigma level in Kron-Cousins I band. At K less than or = 20 the reddest (I-K) color is 5.1 +/- 0.4, and 15 of the 123 objects in the deep field sample have (I-K) greater than 4. In the blue, the galaxies show a rapid blueward trend at magnitudes beyond K = 19, dropping from a median (B-K) = 6 at K = 18 to a median (B-K) of only 4.2 at K = 21.5. The surface density of (I-K) greater than 4 objects is interpreted to imply either that there is a significant evolution toward later types in the colors of the normal galaxy population beyond z = 11 or that galaxies have faded by that redshift.
Document ID
19950050295
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Cowie, L. L.
(Univ. of Hawaii, Honolulu, HI United States)
Gardner, J. P.
(Univ. of Hawaii, Honolulu, HI United States)
Hu, E. M.
(Univ. of Hawaii, Honolulu, HI United States)
Songaila, A.
(Univ. of Hawaii, Honolulu, HI United States)
Hodapp, K.-W.
(Univ. of Hawaii, Honolulu, HI United States)
Wainscoat, R. J.
(Univ. of Hawaii, Honolulu, HI United States)
Date Acquired
August 16, 2013
Publication Date
October 10, 1994
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 434
Issue: 1
ISSN: 0004-637X
Subject Category
Astronomy
Accession Number
95A81894
Funding Number(s)
CONTRACT_GRANT: NAGW-959
Distribution Limits
Public
Copyright
Other

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