A deep wide-field, optical, and near-infrared catalog of a large area around the Hubble Deep Field North

被引:285
作者
Capak, P
Cowie, LL
Hu, EM
Barger, AJ
Dickinson, M
Fernandez, E
Giavalisco, M
Komiyama, Y
Kretchmer, C
McNally, C
Miyazaki, S
Okamura, S
Stern, D
机构
[1] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[2] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA
[3] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA
[4] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[5] New Mexico Inst Min & Technol, Socorro, NM 87801 USA
[6] Subaru Telescope, Hilo, HI 96720 USA
[7] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[8] Univ Maine, Dept Phys & Astron, Orono, ME 04469 USA
[9] Univ Tokyo, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
[10] Univ Tokyo, Res Ctr Early Universe, Bunkyo Ku, Tokyo 1130033, Japan
[11] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
cosmology : observations; galaxies : evolution;
D O I
10.1086/380611
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have conducted a deep multicolor imaging survey of 0.2 deg(2) centered on the Hubble Deep Field North (HDF-N). We shall refer to this region as the Hawaii HDF-N. Deep data were collected in U, B, V, R, I, and z' bands over the central 0.2 deg(2) and in HK' over a smaller region covering the Chandra Deep Field North. The data were reduced to have accurate relative photometry and astrometry across the entire field to facilitate photometric redshifts and spectroscopic follow-up. We have compiled a catalog of 48,858 objects in the central 0.2 deg(2) detected at 5 sigma significance in a 3" aperture in either R or z' band. Number counts and color-magnitude diagrams are presented and shown to be consistent with previous observations. Using color selection we have measured the density of objects at 3<z<7. Our multicolor data indicates that samples selected at z>5.5 using the Lyman break technique suffer from more contamination by low-redshift objects than suggested by previous studies.
引用
收藏
页码:180 / 198
页数:19
相关论文
共 44 条
[1]   Optical and infrared properties of the 2 Ms Chandra Deep Field North X-ray sources [J].
Barger, AJ ;
Cowie, LL ;
Capak, P ;
Alexander, DM ;
Bauer, FE ;
Fernandez, E ;
Brandt, WN ;
Garmire, GP ;
Hornschemeier, AE .
ASTRONOMICAL JOURNAL, 2003, 126 (02) :632-665
[2]   X-ray, optical, and infrared imaging and spectral properties of the 1 Ms Chandra Deep Field North sources [J].
Barger, AJ ;
Cowie, LL ;
Brandt, WN ;
Capak, P ;
Garmire, GP ;
Hornschemeier, AE ;
Steffen, AT ;
Wehner, EH .
ASTRONOMICAL JOURNAL, 2002, 124 (04) :1839-1885
[3]   Bayesian photometric redshift estimation [J].
Benítez, N .
ASTROPHYSICAL JOURNAL, 2000, 536 (02) :571-583
[4]   Near-infrared galaxy counts to J and K∼24 as a function of image size [J].
Bershady, MA ;
Lowenthal, JD ;
Koo, DC .
ASTROPHYSICAL JOURNAL, 1998, 505 (01) :50-73
[5]   SExtractor: Software for source extraction [J].
Bertin, E ;
Arnouts, S .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1996, 117 (02) :393-404
[6]  
BROWN GS, 1974, ASTROPHYS J, V194, P555, DOI 10.1086/153274
[7]  
CAPAK P, 2004, UNPUB
[8]   Caltech faint galaxy redshift survey. X. A redshift survey in the region of the Hubble Deep Field North [J].
Cohen, JG ;
Hogg, DW ;
Blandford, R ;
Cowie, LL ;
Hu, E ;
Songaila, A ;
Shopbell, P ;
Richberg, K .
ASTROPHYSICAL JOURNAL, 2000, 538 (01) :29-52
[9]   COLORS AND MAGNITUDES PREDICTED FOR HIGH REDSHIFT GALAXIES [J].
COLEMAN, GD ;
WU, CC ;
WEEDMAN, DW .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1980, 43 (03) :393-416
[10]  
Cowie L. L., 1988, POST RECOMBINATION U, P1