An AzTEC 1.1 mm survey of the GOODS-N field - I. Maps, catalogue and source statistics

被引:105
作者
Perera, T. A. [1 ]
Chapin, E. L. [2 ]
Austermann, J. E. [1 ]
Scott, K. S. [1 ]
Wilson, G. W. [1 ]
Halpern, M. [2 ]
Pope, A. [2 ,3 ]
Scott, D. [2 ]
Yun, M. S. [1 ]
Lowenthal, J. D. [4 ]
Morrison, G. [5 ,6 ]
Aretxaga, I. [7 ]
Bock, J. J. [8 ]
Coppin, K. [9 ]
Crowe, M. [2 ]
Frey, L. [2 ]
Hughes, D. H. [7 ]
Kang, Y. [10 ]
Kim, S. [10 ]
Mauskopf, P. D. [11 ]
机构
[1] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
[2] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[3] Natl Opt Astron Observ, Tucson, AZ 85719 USA
[4] Smith Coll, Dept Astron, Northampton, MA 01063 USA
[5] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[6] Canada France Hawaii Telescope Corp, Kamuela, HI 96743 USA
[7] Inst Nacl Astrofis Opt & Electr, Puebla, Mexico
[8] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[9] Univ Durham, Inst Computat Cosmol, Durham DH1 3LE, England
[10] Sejong Univ, Dept Astron & Space Sci, Seoul, South Korea
[11] Cardiff Univ, Cardiff, S Glam, Wales
基金
英国科学技术设施理事会; 加拿大自然科学与工程研究理事会;
关键词
instrumentation: detectors; galaxies: high redshift; galaxies: starburst; submillimetre;
D O I
10.1111/j.1365-2966.2008.13902.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have conducted a deep and uniform 1.1 mm survey of the Great Observatories Origins Deep Survey-North (GOODS-N) field with AzTEC on the James Clerk Maxwell Telescope. Here, we present the first results from this survey including maps, the source catalogue and 1.1 mm number counts. The results presented here were obtained from a 245 arcmin(2) region with a near uniform coverage to a depth of 0.96-1.16 mJy beam(-1). Our robust catalogue contains 28 source candidates detected with S/N >= 3.75, only similar to 1-2 of which are expected to be spurious detections. Of these source candidates, eight are also detected by Submillimetre Common-User Bolometer Array ( SCUBA) at 850 mu m in regions where there is a good overlap between the two surveys. The major advantage of our survey over that with SCUBA is the uniformity of coverage. We calculate number counts using two different techniques: the first using a frequentist parameter estimation and the second using a Bayesian method. The two sets of results are in good agreement. We find that the 1.1 mm differential number counts are well described in the 2-6 mJy range by the functional form dN/dS = N'(S'/S) exp(-S/S') with fitted parameters S' = 1.25 +/- 0.38 mJy and dN/dS = 300 +/- 90 mJy(-1) deg(-2) at 3 mJy.
引用
收藏
页码:1227 / 1238
页数:12
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