The Bright Ages Survey. I. Imaging Data
Autor: | Samir Salim, R. Michael Rich, Jay A. Frogel, Harry I. Teplitz, James Colbert, Matthew A. Malkan |
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Rok vydání: | 2006 |
Předmět: |
Field (physics)
FOS: Physical sciences Astrophysics Astronomy & Astrophysics Physical Chemistry galaxies [infrared] Atomic 01 natural sciences Imaging data Particle and Plasma Physics astro-ph 0103 physical sciences Nuclear 010303 astronomy & astrophysics evolution [galaxies] Physics Number density 010308 nuclear & particles physics Astrophysics (astro-ph) Molecular Astronomy and Astrophysics Cosmic variance Redshift Galaxy Space and Planetary Science high-redshift [galaxies] Astronomical and Space Sciences Physical Chemistry (incl. Structural) |
Zdroj: | Colbert, JW; Malkan, MA; Rich, RM; Frogel, JA; Salim, S; & Teplitz, H. (2006). The bright ages survey. I. Imaging data. Astrophysical Journal, 638(2 I), 603-612. doi: 10.1086/499095. UCLA: Retrieved from: http://www.escholarship.org/uc/item/7v19d3sf The Astrophysical Journal, vol 638, iss 2 Astrophysical Journal, vol 638, iss 2 I |
ISSN: | 1538-4357 0004-637X |
DOI: | 10.1086/499095 |
Popis: | This is the first paper in a series presenting and analyzing data for a K-selected sample of galaxies collected in order to identify and study galaxies at moderate to high redshift in rest-wavelength optical light. The sample contains 842 objects over 6 separate fields covering 75.6 arcmin^2 down to K=20-20.5. We combine the K-band with UBVRIzJH multi-band imaging, reaching depths of R~26. Two of the fields studied also have deep HST WFPC2 imaging, totaling more than 60 hours in the F300W, F450W, F606W, and F814W filters. Using artificial galaxy modeling and extraction we measure 85% completeness limits down to K=19.5-20, depending on the field examined. The derived K-band number counts are in good agreement with previous studies. We find a density for Extremely Red Objects(EROs; R-K>5) of 1.55+/-0.16 arcmin^{-2} for K 30 pages, 5 figures, accepted by ApJ |
Databáze: | OpenAIRE |
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