Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours

被引:106
作者
Amblard, A. [1 ]
Cooray, A. [1 ]
Serra, P. [1 ]
Temi, P. [2 ]
Barton, E. [1 ]
Negrello, M. [3 ]
Auld, R. [4 ]
Baes, M. [5 ]
Baldry, I. K. [6 ]
Bamford, S. [7 ]
Blain, A.
Bock, J. [8 ,9 ]
Bonfield, D. [10 ]
Burgarella, D. [11 ]
Buttiglione, S. [12 ]
Cameron, E. [13 ]
Cava, A. [14 ,15 ]
Clements, D. [16 ]
Croom, S. [17 ]
Dariush, A. [4 ]
de Zotti, G. [12 ,22 ]
Driver, S. [18 ]
Dunlop, J. [19 ]
Dunne, L. [7 ]
Dye, S. [4 ]
Eales, S. [4 ]
Frayer, D. [20 ]
Fritz, J. [5 ]
Gardner, Jonathan P. [21 ]
Gonzalez-Nuevo, J. [22 ]
Herranz, D. [23 ]
Hill, D. [18 ]
Hopkins, A. [24 ]
Hughes, D. H. [25 ]
Ibar, E. [26 ]
Ivison, R. J. [26 ]
Jarvis, M. [10 ]
Jones, D. H. [24 ]
Kelvin, L. [18 ]
Lagache, G. [38 ,39 ,40 ]
Leeuw, L. [2 ]
Liske, J. [27 ]
Lopez-Caniego, M. [23 ]
Loveday, J. [28 ]
Maddox, S. [7 ]
Michalowski, M. [19 ]
Norberg, P. [19 ]
Parkinson, H. [19 ]
Peacock, J. A. [19 ]
Pearson, C. [36 ,37 ]
机构
[1] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
[2] NASA, Ames Res Ctr, Astrophys Branch, Moffett Field, CA 94035 USA
[3] Open Univ, Dept Phys & Astron, Milton Keynes MK7 6AA, Bucks, England
[4] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales
[5] Univ Ghent, Sterrenkundig Observatorium, B-9000 Ghent, Belgium
[6] Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Merseyside, England
[7] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England
[8] CALTECH, Dept Astron, Pasadena, CA 91125 USA
[9] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[10] Univ Hertfordshire, Sci & Technol Res Ctr, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England
[11] CNRS, UMR6110, Lab Astrophys Marseille, F-13388 Marseille, France
[12] Osserv Astron Padova, INAF, I-35122 Padua, Italy
[13] ETH, Insitute Astron, CH-8093 Zurich, Switzerland
[14] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Spain
[15] Univ La Laguna, Dept Astrofis, Tenerife 38205, Spain
[16] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England
[17] Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia
[18] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland
[19] Univ Edinburgh, Scottish Univ Phys Alliance, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
[20] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA
[21] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[22] Scuola Int Super Studi Avanzati, I-34151 Trieste, Italy
[23] Inst Fis Cantabria CSIC UC, Santander 39005, Spain
[24] Anglo Australian Observ, Epping, NSW 1710, Australia
[25] INAOE, Puebla 72840, Mexico
[26] Royal Observ Edinburgh, UK Astron Technol Ctr, Edinburgh EH9 3HJ, Midlothian, Scotland
[27] European So Observ, D-85748 Garching, Germany
[28] Univ Sussex, Ctr Astron, Brighton BN1 9QH, E Sussex, England
[29] Univ Oxford, Oxford Astrophys, Oxford OX1 3RH, England
[30] Leiden Univ, Sterrewacht Leiden, NL-2300 RA Leiden, Netherlands
[31] ESA, ESAC, Herschel Sci Ctr, Madrid 28691, Spain
[32] Max Planck Inst Nucl Astrophys MPIK, D-69117 Heidelberg, Germany
[33] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[34] Univ Padua, Dept Astron, I-35122 Padua, Italy
[35] Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England
[36] Univ Lethbridge, Inst Space Imaging Sci, Lethbridge, AB T1K 3M4, Canada
[37] Rutherford Appleton Lab, Space Sci & Technol Dept CCLRC RAL, Didcot OX11 0QX, Oxon, England
[38] IAS, F-91405 Orsay, France
[39] Univ Paris 11, Orsay, France
[40] CNRS, UMR 8617, F-75700 Paris, France
基金
美国国家科学基金会;
关键词
submillimeter: galaxies; Galaxy: evolution; galaxies: high-redshift; UNIVERSE GALAXY SURVEY; DEGREE EXTRAGALACTIC SURVEY; PHOTOMETRIC REDSHIFTS; COLD DUST; BLAST; HISTORY; RADIO; IV;
D O I
10.1051/0004-6361/201014586
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present colour-colour diagrams of detected sources in the Herschel-ATLAS science demonstration field from 100 to 500 mu m using both PACS and SPIRE. We fit isothermal modified black bodies to the spectral energy distribution (SED) to extract the dust temperature of sources with counterparts in Galaxy And Mass Assembly (GAMA) or SDSS surveys with either a spectroscopic or a photometric redshift. For a subsample of 330 sources detected in at least three FIR bands with a significance greater than 3 sigma, we find an average dust temperature of (28 +/- 8) K. For sources with no known redshift, we populate the colour-colour diagram with a large number of SEDs generated with a broad range of dust temperatures and emissivity parameters, and compare to colours of observed sources to establish the redshift distribution of this sample. For another subsample of 1686 sources with fluxes above 35 mJy at 350 mu m and detected at 250 and 500 mu m with a significance greater than 3s, we find an average redshift of 2.2 +/- 0.6.
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页数:5
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