THE INFRARED PROPERTIES OF SOURCES MATCHED IN THE WISE ALL-SKY AND HERSCHEL ATLAS SURVEYS

被引：10

作者：

Bond, Nicholas A. ^{[1
]}

Benford, Dominic J. ^{[1
]}

Gardner, Jonathan P. ^{[1
]}

Amblard, Alexandre ^{[2
]}

Fleuren, Simone ^{[3
]}

Blain, Andrew W. ^{[4
]}

Dunne, Loretta ^{[5
]}

Smith, Daniel J. B. ^{[6
]}

Maddox, Steve J. ^{[5
]}

Hoyos, Carlos ^{[5
]}

Baes, Maarten ^{[7
]}

Bonfield, David ^{[6
]}

Bourne, Nathan ^{[5
]}

Bridge, Carrie ^{[8
]}

Buttiglione, Sara ^{[9
]}

Cava, Antonio ^{[10
]}

Clements, David ^{[11
]}

Cooray, Asantha ^{[12
]}

Dariush, Ali ^{[13
]}

de Zotti, Gianfranco ^{[9
,14
]}

Driver, Simon ^{[15
,16
]}

Dye, Simon ^{[5
]}

Eales, Steve ^{[17
]}

Eisenhardt, Peter ^{[18
]}

Hopwood, Rosalind ^{[13
]}

Ibar, Edo ^{[19
]}

Ivison, Rob J. ^{[19
]}

Jarvis, Matt J. ^{[6
,20
]}

Kelvin, Lee ^{[15
,16
]}

Robotham, Aaron S. G. ^{[15
,16
]}

Temi, Pasquale ^{[2
]}

Thompson, Mark ^{[6
]}

Tsai, Chao-Wei ^{[21
]}

van der Werf, Paul ^{[22
]}

Wright, Edward L. ^{[23
]}

Wu, Jingwen ^{[16
]}

Yan, Lin ^{[24
]}

机构：

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

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

[3] Univ London, Sch Math Sci, London E1 4NS, England

[4] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England

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

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

[7] Univ Ghent, Sterrenkundig Observ, B-9000 Ghent, Belgium

[8] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA

[9] Osserv Astron Padova, INAF, I-35122 Padua, Italy

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

[11] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England

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

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

[14] SISSA, I-34136 Trieste, Italy

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

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

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

[18] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

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

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

[21] CALTECH, IPAC, Pasadena, CA 91125 USA

[22] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[23] UCLA Astron, Los Angeles, CA 90095 USA

[24] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2012年 / 750卷 / 01期

基金：

美国国家航空航天局; 美国国家科学基金会;

关键词：

cosmology: observations; galaxies: general; galaxies: high-redshift; galaxies: statistics; infrared: galaxies; surveys; ACTIVE GALACTIC NUCLEI; STAR-FORMING GALAXIES; REDSHIFT SURVEY; DATA RELEASE; SUBMILLIMETER; PERFORMANCE; POPULATION; TELESCOPE; EVOLUTION; SELECTION;

D O I：

10.1088/2041-8205/750/1/L18

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe the infrared properties of sources detected over similar to 36 deg(2) of sky in the GAMA 15 hr equatorial field, using data from both the Herschel Astrophysical Terahertz Large-Area Survey (H-ATLAS) and Wide-field Infrared Survey (WISE). With 5 sigma point-source depths of 34 and 0.048 mJy at 250 mu m and 3.4 mu m, respectively, we are able to identify 50.6% of the H-ATLAS sources in the WISE survey, corresponding to a surface density of similar to 630 deg(-2). Approximately two-thirds of these sources have measured spectroscopic or optical/near-IR photometric redshifts of z < 1. For sources with spectroscopic redshifts at z < 0.3, we find a linear correlation between the infrared luminosity at 3.4 mu m and that at 250 mu m, with +/- 50% scatter over similar to 1.5 orders of magnitude in luminosity, similar to 10(9)-10(10.5) L-circle dot. By contrast, the matched sources without previously measured redshifts (r greater than or similar to 20.5) have 250-350 mu m flux density ratios which suggest either high-redshift galaxies (z greater than or similar to 1.5) or optically faint low-redshift galaxies with unusually low temperatures (T less than or similar to 20). Their small 3.4-250 mu m flux ratios favor a high-redshift galaxy population, as only the most actively star-forming galaxies at low redshift (e.g., Lambda rp 220) exhibit comparable flux density ratios. Furthermore, we find a relatively large active galactic nucleus fraction (similar to 30%) in a 12 mu m flux-limited subsample of H-ATLAS sources, also consistent with there being a significant population of high-redshift sources in the no-redshift sample.

引用

页数：6

共 40 条

[1] THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
Abazajian, Kevork N.
Adelman-McCarthy, Jennifer K.
Agueros, Marcel A.
Allam, Sahar S.
Prieto, Carlos Allende
An, Deokkeun
Anderson, Kurt S. J.
Anderson, Scott F.
Annis, James
Bahcall, Neta A.
Bailer-Jones, C. A. L.
Barentine, J. C.
Bassett, Bruce A.
Becker, Andrew C.
Beers, Timothy C.
Bell, Eric F.
Belokurov, Vasily
Berlind, Andreas A.
Berman, Eileen F.
Bernardi, Mariangela
Bickerton, Steven J.
Bizyaev, Dmitry
Blakeslee, John P.
Blanton, Michael R.
Bochanski, John J.
Boroski, William N.
Brewington, Howard J.
Brinchmann, Jarle
Brinkmann, J.
Brunner, Robert J.
Budavari, Tamas
Carey, Larry N.
Carliles, Samuel
Carr, Michael A.
Castander, Francisco J.
Cinabro, David
Connolly, A. J.
Csabai, Istvan
Cunha, Carlos E.
Czarapata, Paul C.
Davenport, James R. A.
de Haas, Ernst
Dilday, Ben
Doi, Mamoru
Eisenstein, Daniel J.
Evans, Michael L.
Evans, N. W.
Fan, Xiaohui
Friedman, Scott D.
Frieman, Joshua A.
[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2009, 182 (02) : 543 - 558
[2] Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours
Amblard, A.
Cooray, A.
Serra, P.
Temi, P.
Barton, E.
Negrello, M.
Auld, R.
Baes, M.
Baldry, I. K.
Bamford, S.
Blain, A.
Bock, J.
Bonfield, D.
Burgarella, D.
Buttiglione, S.
Cameron, E.
Cava, A.
Clements, D.
Croom, S.
Dariush, A.
de Zotti, G.
Driver, S.
Dunlop, J.
Dunne, L.
Dye, S.
Eales, S.
Frayer, D.
Fritz, J.
Gardner, Jonathan P.
Gonzalez-Nuevo, J.
Herranz, D.
Hill, D.
Hopkins, A.
Hughes, D. H.
Ibar, E.
Ivison, R. J.
Jarvis, M.
Jones, D. H.
Kelvin, L.
Lagache, G.
Leeuw, L.
Liske, J.
Lopez-Caniego, M.
Loveday, J.
Maddox, S.
Michalowski, M.
Norberg, P.
Parkinson, H.
Peacock, J. A.
Pearson, C.
[J]. ASTRONOMY & ASTROPHYSICS, 2010, 518
[3] A redshift survey of the submillimeter galaxy population
Chapman, SC
Blain, AW
Smail, I
Ivison, RJ
[J]. ASTROPHYSICAL JOURNAL, 2005, 622 (02) : 772 - 796
[4] MID-INFRARED SPECTROSCOPY OF CANDIDATE ACTIVE GALACTIC NUCLEI-DOMINATED SUBMILLIMETER GALAXIES
Coppin, K.
Pope, A.
Menendez-Delmestre, K.
Alexander, D. M.
Dunlop, J. S.
Egami, E.
Gabor, J.
Ibar, Edo
Ivison, R. J.
Austermann, J. E.
Blain, A. W.
Chapman, S. C.
Clements, D. L.
Dunne, L.
Dye, S.
Farrah, D.
Hughes, D. H.
Mortier, A. M. J.
Page, M. J.
Rowan-Robinson, M.
Scott, D.
Simpson, C.
Smail, Ian
Swinbank, A. M.
Vaccari, M.
Yun, M. S.
[J]. ASTROPHYSICAL JOURNAL, 2010, 713 (01) : 503 - 519
[5] Multiwavelength study of massive galaxies at z ∼ 2.: I.: Star formation and galaxy growth
Daddi, E.
Dickinson, M.
Morrison, G.
Chary, R.
Cimatti, A.
Elbaz, D.
Frayer, D.
Renzini, A.
Pope, A.
Alexander, D. M.
Bauer, F. E.
Giavalisco, M.
Huynh, M.
Kurk, J.
Mignoli, M.
[J]. ASTROPHYSICAL JOURNAL, 2007, 670 (01) : 156 - 172
[6] IDENTIFYING LUMINOUS ACTIVE GALACTIC NUCLEI IN DEEP SURVEYS: REVISED IRAC SELECTION CRITERIA
Donley, J. L.
Koekemoer, A. M.
Brusa, M.
Capak, P.
Cardamone, C. N.
Civano, F.
Ilbert, O.
Impey, C. D.
Kartaltepe, J. S.
Miyaji, T.
Salvato, M.
Sanders, D. B.
Trump, J. R.
Zamorani, G.
[J]. ASTROPHYSICAL JOURNAL, 2012, 748 (02)
[7] ORIGIN OF 12 μm EMISSION ACROSS GALAXY POPULATIONS FROM WISE AND SDSS SURVEYS
Donoso, E.
Yan, Lin
Tsai, C.
Eisenhardt, P.
Stern, D.
Assef, R. J.
Leisawitz, D.
Jarrett, T. H.
Stanford, S. A.
[J]. ASTROPHYSICAL JOURNAL, 2012, 748 (02)
[8] Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release
Driver, S. P.
Hill, D. T.
Kelvin, L. S.
Robotham, A. S. G.
Liske, J.
Norberg, P.
Baldry, I. K.
Bamford, S. P.
Hopkins, A. M.
Loveday, J.
Peacock, J. A.
Andrae, E.
Bland-Hawthorn, J.
Brough, S.
Brown, M. J. I.
Cameron, E.
Ching, J. H. Y.
Colless, M.
Conselice, C. J.
Croom, S. M.
Cross, N. J. G.
De Propris, R.
Dye, S.
Drinkwater, M. J.
Ellis, S.
Graham, Alister W.
Grootes, M. W.
Gunawardhana, M.
Jones, D. H.
van Kampen, E.
Maraston, C.
Nichol, R. C.
Parkinson, H. R.
Phillipps, S.
Pimbblet, K.
Popescu, C. C.
Prescott, M.
Roseboom, I. G.
Sadler, E. M.
Sansom, A. E.
Sharp, R. G.
Smith, D. J. B.
Taylor, E.
Thomas, D.
Tuffs, R. J.
Wijesinghe, D.
Dunne, L.
Frenk, C. S.
Jarvis, M. J.
Madore, B. F.
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 413 (02) : 971 - 995
[9] Herschel -ATLAS: rapid evolution of dust in galaxies over the last 5 billion years
Dunne, L.
Gomez, H. L.
da Cunha, E.
Charlot, S.
Dye, S.
Eales, S.
Maddox, S. J.
Rowlands, K.
Smith, D. J. B.
Auld, R.
Baes, M.
Bonfield, D. G.
Bourne, N.
Buttiglione, S.
Cava, A.
Clements, D. L.
Coppin, K. E. K.
Cooray, A.
Dariush, A.
de Zotti, G.
Driver, S.
Fritz, J.
Geach, J.
Hopwood, R.
Ibar, E.
Ivison, R. J.
Jarvis, M. J.
Kelvin, L.
Pascale, E.
Pohlen, M.
Popescu, C.
Rigby, E. E.
Robotham, A.
Rodighiero, G.
Sansom, A. E.
Serjeant, S.
Temi, P.
Thompson, M.
Tuffs, R.
van der Werf, P.
Vlahakis, C.
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2011, 417 (02) : 1510 - 1533
[10] Herschel-ATLAS: Evolution of the 250 μm luminosity function out to z = 0.5
Dye, S.
Dunne, L.
Eales, S.
Smith, D. J. B.
Amblard, A.
Auld, R.
Baes, M.
Baldry, I. K.
Bamford, S.
Blain, A. W.
Bonfield, D. G.
Bremer, M.
Burgarella, D.
Buttiglione, S.
Cameron, E.
Cava, A.
Clements, D. L.
Cooray, A.
Croom, S.
Dariush, A.
de Zotti, G.
Driver, S.
Dunlop, J. S.
Frayer, D.
Fritz, J.
Gardner, Jonathan P.
Gomez, H. L.
Gonzalez-Nuevo, J.
Herranz, D.
Hill, D.
Hopkins, A.
Ibar, E.
Ivison, R. J.
Jarvis, M. J.
Jones, D. H.
Kelvin, L.
Lagache, G.
Leeuw, L.
Liske, J.
Lopez-Caniego, M.
Loveday, J.
Maddox, S.
Michalowski, M. J.
Negrello, M.
Norberg, P.
Page, M. J.
Parkinson, H.
Pascale, E.
Peacock, J. A.
Pohlen, M.
[J]. ASTRONOMY & ASTROPHYSICS, 2010, 518

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