Deep atlas radio observations of the Chandra Deep Field-South/Spitzer wide-area infrared extragalactic field

被引:165
作者
Norris, Ray P.
Afonso, Jose
Appleton, Phil N.
Boyle, Brian J.
Ciliegi, Paolo
Croom, Scott M.
Huynh, Minh T.
Jackson, Carole A.
Koekemoer, Anton M.
Lonsdale, Carol J.
Middelberg, Enno
Mobasher, Bahram
Oliver, Seb J.
Polletta, Mari
Siana, Brian D.
Smail, Ian
Voronkov, Maxim A.
机构
[1] CSIRO Australia Telescope, CSIRO Radiophys Lab, Epping, NSW 1710, Australia
[2] Univ Lisbon, Fac Ciencias, Observ Astron Lisboa, P-1349018 Lisbon, Portugal
[3] Univ Lisbon, Ctr Astron & Astrofis, P-1349018 Lisbon, Portugal
[4] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA
[5] Osservatorio Astron Bologna, INAF, I-40127 Bologna, Italy
[6] Anglo Australian Observ, Epping, NSW 1710, Australia
[7] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[8] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
[9] Univ Sussex, Ctr Astron, CPES, Brighton BN1 9QJ, E Sussex, England
[10] Univ Durham, Inst Computat Cosmol, Durham DH1 3LE, England
关键词
catalogs; galaxies : active; galaxies : evolution; radio continuum : galaxies; surveys;
D O I
10.1086/508275
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first results from the Australia Telescope Large Area Survey, which consists of deep radio observations of a 3.7 deg(2) field surrounding the Chandra Deep Field-South, largely coincident with the infrared Spitzer Wide-Area Infrared Extragalactic (SWIRE) Survey. We also list cross-identifications to infrared and optical photometry data from SWIRE, and ground-based optical spectroscopy. A total of 784 radio components are identified, corresponding to 726 distinct radio sources, nearly all of which are identified with SWIRE sources. Of the radio sources with measured redshifts, most lie in the redshift range 0.5-2 and include both star-forming galaxies and active galactic nuclei. We identify a rare population of infrared-faint radio sources that are bright at radio wavelengths but are not seen in the available optical, infrared, or X-ray data. Such rare classes of sources can only be discovered in wide, deep surveys such as this.
引用
收藏
页码:2409 / 2423
页数:15
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