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Constraints on the Early Formation of Field Elliptical Galaxies
Author(s) -
A. J. Barger,
L. L. Cowie,
Neil Trentham,
E. Fulton,
E. M. Hu,
A. Songaila,
Donald N. B. Hall
Publication year - 1999
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/300675
Subject(s) - hubble deep field , elliptical galaxy , hubble ultra deep field , galaxy , redshift , astrophysics , field galaxy , field (mathematics) , physics , population , redshift survey , galaxy formation and evolution , astronomy , mathematics , demography , sociology , pure mathematics
We present the results of an HK' wide-field survey encompassing the HubbleDeep Field and its Flanking Fields. Our wide-field survey provides uniformcoverage of an area 61.8 square arcmin to a depth equivalent to K=20.1 at5-sigma. We have also imaged the Hubble Deep Field in HK', providing uniformcoverage of an area 7.8 square arcmin to a depth equivalent to K=21.2 at5-sigma. Using these data in combination with new deep UH 8K V and I imagingobtained on the CFHT, we find only a small population of objects with colorsredder than an equivalent I-K=4, the color expected for an evolved ellipticalat z>1. We infer that only a fraction of the local field elliptical populationwith M_K<-23.4 could have formed in single bursts at high redshift.Comment: 20 pages, to appear in the Jan 1999 issue of The Astronomical Journa

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