Published June 21, 1997 | Version Published + Accepted Version
Journal Article Open

Counts and colours of faint galaxies in the U and R bands

Abstract

Ground-based counts and colours of faint galaxies in the U and R bands in one field at high Galactic latitude are presented. Integrated over flux, a total of 1.2 × 10^5 source deg^(−2) are found to U = 25.5 mag and 6.3 × 10^5 source deg^(−2) to R = 27 mag, with d log N/dm ∼ 0.5 in the U band and d log N/dm ∼ 0.3 in the R band. Consistent with these number-magnitude curves, sources become bluer with increasing magnitude to median U— R= 0.6 mag at 24

Additional Information

© 1997 RAS. Accepted 1997 February 15. Received 1997 February 5; in original form 1996 April 15. We are grateful to the W. M. Keck Foundation for the vision to fund the construction of the W. M. Keck Observatory. We benefited from helpful conversations with Kurt Adelberger, John Gizis, Tomislav Kundic, Gerry Neugebauer, Sterl Phinney and Chuck Steidel, and from comments from an anonymous referee. We are grateful for financial support from NSF grant AST 92-23370 (DWH, RB), NSF grant AST-91-57412 and the Bressler Foundation (MAP), support through a PPARC Advanced Fellowship (IS), and grants from NSF and NASA (BTS). The calibrated images used for this investigation will be made available to the public; contact the authors for more information. This work is based on observations obtained at the W. M. Keck Observatory, which is operated jointly by the California Institute of Technology and the University of California; and at the Palomar Observatory, which is owned and operated by the California Institute of Technology.

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Published - 288-2-404.pdf

Accepted Version - 9702241

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Additional details

Identifiers

Eprint ID
95755
Resolver ID
CaltechAUTHORS:20190523-125439368

Funding

W. M. Keck Foundation
NSF
AST 92-23370
NSF
AST 91-57412
Bressler Foundation
Particle Physics and Astronomy Research Council (PPARC)
NASA

Dates

Created
2019-05-23
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Updated
2021-11-16
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Physics Department