Herschel-ATLAS: VISTA VIKING near-infrared counterparts in the Phase 1 GAMA 9-h data

被引：32

作者：

Fleuren, S. ^{[1
]}

Sutherland, W. ^{[1
]}

Dunne, L. ^{[2
]}

Smith, D. J. B. ^{[3
]}

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

Gonzalez-Nuevo, J. ^{[4
]}

Findlay, J. ^{[1
]}

Auld, R. ^{[5
]}

Baes, M. ^{[6
]}

Bond, N. A. ^{[7
]}

Bonfield, D. G. ^{[3
]}

Bourne, N. ^{[8
]}

Cooray, A. ^{[9
]}

Buttiglione, S. ^{[10
]}

Cava, A. ^{[11
]}

Dariush, A. ^{[12
]}

De Zotti, G. ^{[4
,10
]}

Driver, S. P. ^{[13
,14
]}

Dye, S. ^{[8
]}

Eales, S. ^{[5
]}

Fritz, J. ^{[6
]}

Gunawardhana, M. L. P. ^{[15
,16
]}

Hopwood, R. ^{[12
,17
]}

Ibar, E. ^{[18
]}

Ivison, R. J. ^{[18
,19
]}

Jarvis, M. J. ^{[3
,20
]}

Kelvin, L. ^{[13
,14
]}

Lapi, A. ^{[4
,21
]}

Liske, J. ^{[22
]}

Michalowski, M. J. ^{[23
]}

Negrello, M. ^{[10
,17
]}

Pascale, E. ^{[5
]}

Pohlen, M. ^{[5
]}

Prescott, M. ^{[24
]}

Rigby, E. E. ^{[23
]}

Robotham, A. ^{[13
]}

Scott, D. ^{[25
]}

Temi, P. ^{[26
]}

Thompson, M. A. ^{[3
]}

Valiante, E. ^{[5
]}

van der Werf, P. ^{[27
]}

机构：

[1] Queen Mary Univ London, Sch Phys & Astron, London E1 4NS, England

[2] Univ Canterbury, Dept Phys & Astron, Christchurch 8140, New Zealand

[3] Univ Hertfordshire, Ctr Astrophys Res, Sci & Technol Res Inst, Hatfield AL10 9AB, Herts, England

[4] SISSA ISAS, Astrophys Sect, I-34136 Trieste, Italy

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

[6] Univ Ghent, Sterrenkundig Observatorium, B-9000 Ghent, Belgium

[7] NASA, Goddard Space Flight Ctr, Cosmol Lab Code 665, Greenbelt, MD 20771 USA

[8] Univ Nottingham, Sch Phys & Astron, Ctr Astron & Particle Theory, Nottingham NG7 1HR, England

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

[10] INAF Osservatorio Astron Padova, I-35122 Padua, Italy

[11] Univ Complutense Madrid, Fac CC Fis, Dept Astrofis, E-28040 Madrid, Spain

[12] Univ London Imperial Coll Sci Technol & Med, Dept Phys, London SW7 2AZ, England

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

[14] Univ Western Australia, ICRAR, Crawley, WA 6009, Australia

[15] Australian Astron Observ, Epping, NSW 1710, Australia

[16] Univ Sydney, Sydney Inst Astron, Sch Phys, Sydney, NSW 2006, Australia

[17] Open Univ, Dept Phys & Astron, Milton Keynes MK7 6AA, Bucks, England

[18] Royal Observ, UK Astron Technol Ctr, Edinburgh EH9 3HJ, Midlothian, Scotland

[19] Univ Edinburgh, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland

[20] Univ Western Cape, Dept Phys, ZA-7535 Cape Town, South Africa

[21] Univ Tor Vergata, Dipartmento Fis, I-00133 Rome, Italy

[22] European So Observ, D-85748 Garching, Germany

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

[24] Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Merseyside, England

[25] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada

[26] NASA, Ames Res Ctr, Astrophys Branch, Moffett Field, CA 94035 USA

[27] Leiden Observ, NL-2300 RA Leiden, Netherlands

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2012年 / 423卷 / 03期

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

methods: statistical; infrared: galaxies; submillimetre: galaxies; DEGREE EXTRAGALACTIC SURVEY; DEEP-FIELD; MERGER RATE; WIDE-FIELD; MIDINFRARED COUNTERPARTS; SUBMILLIMETER GALAXIES; RADIO CORRELATION; REDSHIFT SURVEY; SKY SURVEY; MU-M;

D O I：

10.1111/j.1365-2966.2012.21048.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We identify near-infrared Ks-band counterparts to Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) submillimetre (submm) sources, using a preliminary object catalogue from the VISTA Kilo-degree Infrared Galaxy (VIKING) survey. The submm sources are selected from the H-ATLAS Phase 1 catalogue of the Galaxy and Mass Assembly 9-h field, which includes all objects detected at 250, 350 or with the instrument. We apply and discuss a likelihood ratio method for VIKING candidates within a search radius of 10 arcsec of the 22 000 SPIRE sources with a 5s detection at . We estimate the fraction of SPIRE sources with a counterpart above the magnitude limit of the VIKING survey to be Q0 similar to 0.73. We find that 11 294 (51 per cent) of the SPIRE sources have a best VIKING counterpart with a reliability R= 0.8, and the false identification rate of these is estimated to be 4.2 per cent. We expect to miss 5 per cent of true VIKING counterparts. There is evidence from Z-J and J-Ks colours that the reliable counterparts to SPIRE galaxies are marginally redder than the field population. We obtain photometric redshifts for 68 per cent of all (non-stellar) VIKING candidates with a median redshift of . We have spectroscopic redshifts for 3147 (28 per cent) of the reliable counterparts from existing redshift surveys. Comparing to the results of the optical identifications supplied with the Phase 1 catalogue, we find that the use of medium-deep near-infrared data improves the identification rate of reliable counterparts from 36 to 51 per cent.

引用

页码：2407 / 2424

页数：18

共 69 条

[31] THERMAL INFRARED AND NONTHERMAL RADIO - REMARKABLE CORRELATION IN DISKS OF GALAXIES [J].

HELOU, G ;

SOIFER, BT ;

ROWANROBINSON, M .

ASTROPHYSICAL JOURNAL, 1985, 298 (01) :L7-L11

[32]

Hewitt P.C., 2006, MNRAS, V367, P454

[33] H-ATLAS: PACS imaging for the Science Demonstration Phase [J].

Ibar, Edo ;

Ivison, R. J. ;

Cava, A. ;

Rodighiero, G. ;

Buttiglione, S. ;

Temi, P. ;

Frayer, D. ;

Fritz, J. ;

Leeuw, L. ;

Baes, M. ;

Rigby, E. ;

Verma, A. ;

Serjeant, S. ;

Mueller, T. ;

Auld, R. ;

Dariush, A. ;

Dunne, L. ;

Eales, S. ;

Maddox, S. ;

Panuzzo, P. ;

Pascale, E. ;

Pohlen, M. ;

Smith, D. ;

de Zotti, G. ;

Vaccari, M. ;

Hopwood, R. ;

Cooray, A. ;

Burgarella, D. ;

Jarvis, M. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 409 (01) :38-47

[34] The SCUBA HAlf degree extragalactic survey - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies [J].

Ivison, R. J. ;

Greve, T. R. ;

Dunlop, J. S. ;

Peacock, J. A. ;

Egami, E. ;

Smail, Ian ;

Ibar, E. ;

van Kampen, E. ;

Aretxaga, I. ;

Babbedge, T. ;

Biggs, A. D. ;

Blain, A. W. ;

Chapman, S. C. ;

Clements, D. L. ;

Coppin, K. ;

Farrah, D. ;

Halpern, M. ;

Hughes, D. H. ;

Jarvis, M. J. ;

Jenness, T. ;

Jones, J. R. ;

Mortier, A. M. J. ;

Oliver, S. ;

Papovich, C. ;

Perez-Gonzalez, P. G. ;

Pope, A. ;

Rawlings, S. ;

Rieke, G. H. ;

Rowan-Robinson, M. ;

Savage, R. S. ;

Scott, D. ;

Seigar, M. ;

Serjeant, S. ;

Simpson, C. ;

Stevens, J. A. ;

Vaccari, M. ;

Wagg, J. ;

Willott, C. J. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2007, 380 (01) :199-228

[35] Herschel and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z=2.3 [J].

Ivison, R. J. ;

Swinbank, A. M. ;

Swinyard, B. ;

Smail, I. ;

Pearson, C. P. ;

Rigopoulou, D. ;

Polehampton, E. ;

Baluteau, J. -P. ;

Barlow, M. J. ;

Blain, A. W. ;

Bock, J. ;

Clements, D. L. ;

Coppin, K. ;

Cooray, A. ;

Danielson, A. ;

Dwek, E. ;

Edge, A. C. ;

Franceschini, A. ;

Fulton, T. ;

Glenn, J. ;

Griffin, M. ;

Isaak, K. ;

Leeks, S. ;

Lim, T. ;

Naylor, D. ;

Oliver, S. J. ;

Page, M. J. ;

Perez Fournon, I. ;

Rowan-Robinson, M. ;

Savini, G. ;

Scott, D. ;

Spencer, L. ;

Valtchanov, I. ;

Vigroux, L. ;

Wright, G. S. .

ASTRONOMY & ASTROPHYSICS, 2010, 518

[36] Herschel-ATLAS: the far-infrared-radio correlation at z < 0.5 [J].

Jarvis, Matt J. ;

Smith, D. J. B. ;

Bonfield, D. G. ;

Hardcastle, M. J. ;

Falder, J. T. ;

Stevens, J. A. ;

Ivison, R. J. ;

Auld, R. ;

Baes, M. ;

Baldry, I. K. ;

Bamford, S. P. ;

Bourne, N. ;

Buttiglione, S. ;

Cava, A. ;

Cooray, A. ;

Dariush, A. ;

de Zotti, G. ;

Dunlop, J. S. ;

Dunne, L. ;

Dye, S. ;

Eales, S. ;

Fritz, J. ;

Hill, D. T. ;

Hopwood, R. ;

Hughes, D. H. ;

Ibar, E. ;

Jones, D. H. ;

Kelvin, L. ;

Lawrence, A. ;

Leeuw, L. ;

Loveday, J. ;

Maddox, S. J. ;

Michalowski, M. J. ;

Negrello, M. ;

Norberg, P. ;

Pohlen, M. ;

Prescott, M. ;

Rigby, E. E. ;

Robotham, A. ;

Rodighiero, G. ;

Scott, D. ;

Sharp, R. ;

Temi, P. ;

Thompson, M. A. ;

van der Werf, P. ;

van Kampen, E. ;

Vlahakis, C. ;

White, G. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2010, 409 (01) :92-101

[37]

Johnston S, 2008, EXP ASTRON, V22, P151, DOI 10.1007/s10686-008-9124-7

[38]

Kim S., 2011, ARXIV11123653

[39] Modelling infrared galaxy evolution using a phenomenological approach [J].

Lagache, G ;

Dole, H ;

Puget, JL .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2003, 338 (03) :555-571

[40] HERSCHEL-ATLAS GALAXY COUNTS AND HIGH-REDSHIFT LUMINOSITY FUNCTIONS: THE FORMATION OF MASSIVE EARLY-TYPE GALAXIES [J].

Lapi, A. ;

Gonzalez-Nuevo, J. ;

Fan, L. ;

Bressan, A. ;

De Zotti, G. ;

Danese, L. ;

Negrello, M. ;

Dunne, L. ;

Eales, S. ;

Maddox, S. ;

Auld, R. ;

Baes, M. ;

Bonfield, D. G. ;

Buttiglione, S. ;

Cava, A. ;

Clements, D. L. ;

Cooray, A. ;

Dariush, A. ;

Dye, S. ;

Fritz, J. ;

Herranz, D. ;

Hopwood, R. ;

Ibar, E. ;

Ivison, R. ;

Jarvis, M. J. ;

Kaviraj, S. ;

Lopez-Caniego, M. ;

Massardi, M. ;

Michallowski, M. J. ;

Pascale, E. ;

Pohlen, M. ;

Rigby, E. ;

Rodighiero, G. ;

Serjeant, S. ;

Smith, D. J. B. ;

Temi, P. ;

Wardlow, J. ;

van der Werf, P. .

ASTROPHYSICAL JOURNAL, 2011, 742 (01)

← 1 2 3 4 5 6 7 →