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The Canada-UK deep submillimeter survey. VII. Optical and near-infrared identifications for the 14 hour field
被引:55
作者:

Webb, TMA
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机构: Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada

Lilly, SJ
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机构: Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada

Clements, DL
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机构: Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada

Eales, S
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机构: Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada

Yun, M
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机构: Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada

Brodwin, M
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机构: Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada

Dunne, L
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机构: Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada

Gear, WK
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机构: Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada
机构:
[1] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 1A1, Canada
[2] Sterrewacht Leiden, NL-233 CA Leiden, Netherlands
[3] ETH Honggerberg, Inst Astron, CH-8093 Zurich, Switzerland
[4] Cardiff Univ, Dept Phys & Astron, Cardiff CF2 3YB, S Glam, Wales
[5] Univ Massachusetts, Dept Astron, Lederle Grad Res Ctr 640, Amherst, MA 01003 USA
关键词:
cosmology : observations;
galaxies : evolution;
galaxies : formation;
galaxies : high-redshift;
submillimeter;
D O I:
10.1086/381217
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present the multiwavelength identifications for 23 sources in the Canada-UK Deep Submillimeter Survey (CUDSS) 14(h) field. The identifications have been selected on the basis of radio and near-infrared data, and we argue that, to our observational limits, both are effective at selecting the correct counterparts of the SCUBA sources. We discuss the properties of these identifications and find that they are very red in near-infrared color, with many classified as extremely red objects, and show disturbed morphologies. Using the entire CUDSS catalog of 50 sources, we use a combination of spectroscopic redshifts (four objects), 1.4 GHz: 850 mum flux ratio redshift estimates (10 objects), and redshift lower limits based on nondetections at 1.4 GHz ( the rest of the sample) to estimate a lower limit on the median redshift of the population of z(med)>1.4. Working from simple models and using the properties of the secure identifications, we discuss general and tentative constraints on the redshift distribution and the expected colors and magnitudes of the entire population.
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页码:680 / 698
页数:19
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