The Herschel - ATLAS Data Release 1-II. Multi-wavelength counterparts to submillimetre sources

被引：82

作者：

Bourne, N. ^{[1
]}

Dunne, L. ^{[1
,2
]}

Maddox, S. J. ^{[1
,2
]}

Dye, S. ^{[3
]}

Furlanetto, C. ^{[3
,4
]}

Hoyos, C. ^{[3
,5
,6
]}

Smith, D. J. B. ^{[7
]}

Eales, S. ^{[2
]}

Smith, M. W. L. ^{[2
]}

Valiante, E. ^{[2
]}

Alpaslan, M. ^{[8
,9
]}

Andrae, E. ^{[10
]}

Baldry, I. K. ^{[11
]}

Cluver, M. E. ^{[12
]}

Cooray, A. ^{[13
]}

Driver, S. P. ^{[8
,9
]}

Dunlop, J. S. ^{[1
]}

Grootes, M. W. ^{[10
]}

Ivison, R. J. ^{[1
,14
]}

Jarrett, T. H. ^{[15
]}

Liske, J. ^{[16
]}

Madore, B. F. ^{[17
]}

Popescu, C. C. ^{[18
]}

Robotham, A. G. ^{[8
,9
]}

Rowlands, K. ^{[8
]}

Seibert, M. ^{[17
]}

Thompson, M. A. ^{[7
]}

Tuffs, R. J. ^{[10
]}

Viaene, S. ^{[19
]}

Wright, A. H. ^{[9
]}

机构：

[1] Univ Edinburgh, Royal Observ, Inst Astron, SUPA, Edinburgh EH9 3HJ, Midlothian, Scotland

[2] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[3] Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England

[4] Minist Educ Brazil, CAPES Fdn, BR-70040020 Brasilia, DF, Brazil

[5] Univ Autonoma Madrid, Dept Fis Teor, Crta Colmenar Viejo,Km 15-600, E-28049 Madrid, Spain

[6] Univ Carlos III Madrid, Dept Fis, Campus Leganes,Avda Univ 30, E-28911 Madrid, Spain

[7] Univ Hertfordshire, Sch Phys Astron & Math, Ctr Astrophys Res, Coll Lane, Hatfield AL10 9AB, Herts, England

[8] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland

[9] Univ Western Australia, Int Ctr Radio Astron ICRAR, Crawley, WA 6009, Australia

[10] Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany

[11] Liverpool John Moores Univ, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England

[12] Univ Western Cape, Robert Sobukwe Rd, ZA-7535 Bellville, South Africa

[13] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[14] ESO, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[15] Univ Cape Town, Dept Astron, Private Bag X3, ZA-7701 Rondebosch, South Africa

[16] Univ Hamburg, Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany

[17] Carnegie Inst Washington, 813 Santa Barbara St, Pasadena, CA 91101 USA

[18] Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England

[19] Univ Ghent, Sterrenkundig Observ, Krijgslaan 281, B-9000 Ghent, Belgium

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2016年 / 462卷 / 02期

基金：

美国国家航空航天局; 美国国家科学基金会; 欧洲研究理事会; 英国科学技术设施理事会;

关键词：

methods: statistical; catalogues; submillimetre: galaxies; submillimetre: stars; MASS ASSEMBLY GAMA; DIGITAL SKY SURVEY; EARLY-TYPE GALAXIES; STAR-FORMATION; REDSHIFT SURVEY; DUST ATTENUATION; 2DF-SDSS LRG; DEBRIS DISKS; ALL-SKY; MU-M;

D O I：

10.1093/mnras/stw1654

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper is the second in a pair of papers presenting data release 1 (DR1) of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), the largest single open-time key project carried out with the Herschel Space Observatory. The H-ATLAS is a wide-area imaging survey carried out in five photometric bands at 100, 160, 250, 350 and 500 mu m covering a total area of 600 deg2. In this paper, we describe the identification of optical counterparts to submillimetre sources in DR1, comprising an area of 161 deg2 over three equatorial fields of roughly 12 x 4.5 deg centred at 9(h), 12(h) and 14.(h)5, respectively. Of all the H-ATLAS fields, the equatorial regions benefit from the greatest overlap with current multi-wavelength surveys spanning ultraviolet (UV) to mid-infrared regimes, as well as extensive spectroscopic coverage. We use a likelihood ratio technique to identify Sloan Digital Sky Survey counterparts at r < 22.4 for 250-mu m-selected sources detected at >= 4 sigma (approximate to 28 mJy). We find 'reliable' counterparts (reliability R >= 0.8) for 44 835 sources (39 per cent), with an estimated completeness of 73.0 per cent and contamination rate of 4.7 per cent. Using redshifts and multi-wavelength photometry from GAMA and other public catalogues, we show that H-ATLAS-selected galaxies at z < 0.5 span a wide range of optical colours, total infrared (IR) luminosities and IR/UV ratios, with no strong disposition towards mid-IR-classified active galactic nuclei in comparison with optical selection. The data described herein, together with all maps and catalogues described in the companion paper, are available from the H-ATLAS website at www.h-atlas.org.

引用

页码：1714 / 1734

页数：21

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