Herschel–ATLAS: counterparts from the ultraviolet–near‐infrared in the science demonstration phase catalogue
Identifieur interne : 000166 ( France/Analysis ); précédent : 000165; suivant : 000167Herschel–ATLAS: counterparts from the ultraviolet–near‐infrared in the science demonstration phase catalogue
Auteurs : D. J. B. Smith ; L. Dunne ; S. J. Maddox ; S. Eales ; D. G. Bonfield ; M. J. Jarvis ; W. Sutherland ; S. Fleuren ; E. E. Rigby ; M. A. Thompson ; I. K. Baldry ; S. Bamford ; S. Buttiglione [Italie] ; A. Cava [Espagne] ; D. L. Clements ; A. Cooray [États-Unis] ; S. Croom [Australie] ; A. Dariush ; G. De Zotti [Italie] ; S. P. Driver [Australie] ; J. S. Dunlop ; J. Fritz [Belgique] ; D. T. Hill ; A. Hopkins [Australie] ; R. Hopwood ; E. Ibar ; R. J. Ivison ; D. H. Jones [Australie] ; L. Kelvin ; L. Leeuw [États-Unis] ; J. Liske [Allemagne] ; J. Loveday ; B. F. Madore [États-Unis] ; P. Norberg ; P. Panuzzo [France] ; E. Pascale ; M. Pohlen ; C. C. Popescu ; M. Prescott ; A. Robotham ; G. Rodighiero [Italie] ; D. Scott [Canada] ; M. Seibert [États-Unis] ; R. Sharp [Australie] ; P. Temi [États-Unis] ; R. J. Tuffs [Allemagne] ; P. Van Der Werf [Pays-Bas] ; E. Van Kampen [Allemagne]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-09-11.
English descriptors
Abstract
We present a technique to identify optical counterparts of 250‐μm‐selected sources from the Herschel–ATLAS survey. Of the 6621 250 μm > 32‐mJy sources in our science demonstration catalogue we find that ∼60 per cent have counterparts brighter than r = 22.4 mag in the Sloan Digital Sky Survey. Applying a likelihood ratio technique we are able to identify 2423 of the counterparts with a reliability R > 0.8. This is approximately 37 per cent of the full 250‐μm catalogue. We have estimated photometric redshifts for each of these 2423 reliable counterparts, while 1099 also have spectroscopic redshifts collated from several different sources, including the GAMA survey. We estimate the completeness of identifying counterparts as a function of redshift, and present evidence that 250‐μm‐selected Herschel–ATLAS galaxies have a bimodal redshift distribution. Those with reliable optical identifications have a redshift distribution peaking at z ≈ 0.25 ± 0.05, while submillimetre colours suggest that a significant fraction with no counterpart above the r‐band limit have z > 1. We also suggest a method for selecting populations of strongly lensed high‐redshift galaxies. Our identifications are matched to UV–NIR photometry from the GAMA survey, and these data are available as part of the Herschel–ATLAS public data release.
Url:
DOI: 10.1111/j.1365-2966.2011.18827.x
Affiliations:
- Allemagne, Australie, Belgique, Canada, Espagne, France, Italie, Pays-Bas, États-Unis
- Bade-Wurtemberg, Californie, Communauté de Madrid, District de Karlsruhe, Province de Flandre-Orientale, Région flamande
- Gand, Heidelberg, Madrid
- Université complutense de Madrid, Université de Gand
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ISTEX:A0DF6586BAE8156157D7A336C1BD91E5D2E6B5C1Le document en format XML
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Dariush</name><affiliation><wicri:noCountry code="subField">3AA</wicri:noCountry></affiliation></author><author><name sortKey="De Zotti, G" sort="De Zotti, G" uniqKey="De Zotti G" first="G." last="De Zotti">G. De Zotti</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>INAF – Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, I‐35122 Padova</wicri:regionArea><wicri:noRegion>I‐35122 Padova</wicri:noRegion></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>SISSA, Via Bonomea 265, I‐34136 Trieste</wicri:regionArea><wicri:noRegion>I‐34136 Trieste</wicri:noRegion></affiliation></author><author><name sortKey="Driver, S P" sort="Driver, S P" uniqKey="Driver S" first="S. P." last="Driver">S. P. Driver</name><affiliation></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Australie</country><wicri:regionArea>International Centre for Radio Astronomy Research, The University of Western Australia, 7 Fairway, Crawley, Perth, Western Australia WA6009</wicri:regionArea><wicri:noRegion>Western Australia WA6009</wicri:noRegion></affiliation></author><author><name sortKey="Dunlop, J S" sort="Dunlop, J S" uniqKey="Dunlop J" first="J. S." last="Dunlop">J. S. Dunlop</name><affiliation><wicri:noCountry code="subField">3HJ</wicri:noCountry></affiliation></author><author><name sortKey="Fritz, J" sort="Fritz, J" uniqKey="Fritz J" first="J." last="Fritz">J. Fritz</name><affiliation wicri:level="4"><country xml:lang="fr">Belgique</country><wicri:regionArea>Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, B‐9000 Gent</wicri:regionArea><orgName type="university">Université de Gand</orgName><placeName><settlement type="city">Gand</settlement><region>Région flamande</region><region type="district" nuts="2">Province de Flandre-Orientale</region></placeName></affiliation></author><author><name sortKey="Hill, D T" sort="Hill, D T" uniqKey="Hill D" first="D. T." last="Hill">D. T. Hill</name><affiliation><wicri:noCountry code="subField">9SS</wicri:noCountry></affiliation></author><author><name sortKey="Hopkins, A" sort="Hopkins, A" uniqKey="Hopkins A" first="A." last="Hopkins">A. Hopkins</name><affiliation wicri:level="1"><country xml:lang="fr">Australie</country><wicri:regionArea>Anglo‐Australian Observatory, PO Box 296, Epping, NSW 1710</wicri:regionArea><wicri:noRegion>NSW 1710</wicri:noRegion></affiliation></author><author><name sortKey="Hopwood, R" sort="Hopwood, R" uniqKey="Hopwood R" first="R." last="Hopwood">R. Hopwood</name><affiliation><wicri:noCountry code="subField">6AA</wicri:noCountry></affiliation></author><author><name sortKey="Ibar, E" sort="Ibar, E" uniqKey="Ibar E" first="E." last="Ibar">E. Ibar</name><affiliation><wicri:noCountry code="subField">3HJ</wicri:noCountry></affiliation></author><author><name sortKey="Ivison, R J" sort="Ivison, R J" uniqKey="Ivison R" first="R. J." last="Ivison">R. J. Ivison</name><affiliation></affiliation><affiliation><wicri:noCountry code="subField">3HJ</wicri:noCountry></affiliation></author><author><name sortKey="Jones, D H" sort="Jones, D H" uniqKey="Jones D" first="D. H." last="Jones">D. H. Jones</name><affiliation wicri:level="1"><country xml:lang="fr">Australie</country><wicri:regionArea>Anglo‐Australian Observatory, PO Box 296, Epping, NSW 1710</wicri:regionArea><wicri:noRegion>NSW 1710</wicri:noRegion></affiliation></author><author><name sortKey="Kelvin, L" sort="Kelvin, L" uniqKey="Kelvin L" first="L." last="Kelvin">L. Kelvin</name><affiliation><wicri:noCountry code="subField">9SS</wicri:noCountry></affiliation></author><author><name sortKey="Leeuw, L" sort="Leeuw, L" uniqKey="Leeuw L" first="L." last="Leeuw">L. Leeuw</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>SETI Institute, 515 N. Whisman Avenue, Mountain View, CA 94043</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Liske, J" sort="Liske, J" uniqKey="Liske J" first="J." last="Liske">J. Liske</name><affiliation wicri:level="1"><country xml:lang="fr">Allemagne</country><wicri:regionArea>European Southern Observatory, Karl‐Schwarzschild‐Strasse 2, D‐85748 Garching bei München</wicri:regionArea><wicri:noRegion>85748 Garching bei München</wicri:noRegion><wicri:noRegion>D‐85748 Garching bei München</wicri:noRegion></affiliation></author><author><name sortKey="Loveday, J" sort="Loveday, J" uniqKey="Loveday J" first="J." last="Loveday">J. Loveday</name><affiliation><wicri:noCountry code="subField">9QH</wicri:noCountry></affiliation></author><author><name sortKey="Madore, B F" sort="Madore, B F" uniqKey="Madore B" first="B. F." last="Madore">B. F. Madore</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Observatories of the Carnegie Institution, 813 Santa Barbera St., Pasadena, CA 91101</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Norberg, P" sort="Norberg, P" uniqKey="Norberg P" first="P." last="Norberg">P. Norberg</name><affiliation><wicri:noCountry code="subField">3HJ</wicri:noCountry></affiliation></author><author><name sortKey="Panuzzo, P" sort="Panuzzo, P" uniqKey="Panuzzo P" first="P." last="Panuzzo">P. Panuzzo</name><affiliation wicri:level="1"><country xml:lang="fr">France</country><wicri:regionArea>CEA, Laboratoire AIM, Irfu/SAp, Orme des Merisiers, F‐91191 Gif‐sur‐Yvette</wicri:regionArea><wicri:noRegion>91191 Gif‐sur‐Yvette</wicri:noRegion><wicri:noRegion>F‐91191 Gif‐sur‐Yvette</wicri:noRegion></affiliation></author><author><name sortKey="Pascale, E" sort="Pascale, E" uniqKey="Pascale E" first="E." last="Pascale">E. Pascale</name><affiliation><wicri:noCountry code="subField">3AA</wicri:noCountry></affiliation></author><author><name sortKey="Pohlen, M" sort="Pohlen, M" uniqKey="Pohlen M" first="M." last="Pohlen">M. Pohlen</name><affiliation><wicri:noCountry code="subField">3AA</wicri:noCountry></affiliation></author><author><name sortKey="Popescu, C C" sort="Popescu, C C" uniqKey="Popescu C" first="C. C." last="Popescu">C. C. Popescu</name><affiliation><wicri:noCountry code="subField">2HE</wicri:noCountry></affiliation></author><author><name sortKey="Prescott, M" sort="Prescott, M" uniqKey="Prescott M" first="M." last="Prescott">M. Prescott</name><affiliation><wicri:noCountry code="subField">1LD</wicri:noCountry></affiliation></author><author><name sortKey="Robotham, A" sort="Robotham, A" uniqKey="Robotham A" first="A." last="Robotham">A. Robotham</name><affiliation><wicri:noCountry code="subField">9SS</wicri:noCountry></affiliation></author><author><name sortKey="Rodighiero, G" sort="Rodighiero, G" uniqKey="Rodighiero G" first="G." last="Rodighiero">G. Rodighiero</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>INAF – Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, I‐35122 Padova</wicri:regionArea><wicri:noRegion>I‐35122 Padova</wicri:noRegion></affiliation></author><author><name sortKey="Scott, D" sort="Scott, D" uniqKey="Scott D" first="D." last="Scott">D. Scott</name><affiliation wicri:level="1"><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Physics and Astronomy, 6224 Agricultural Road, University of British Columbia, Vancouver, BC V6T 1Z1</wicri:regionArea><wicri:noRegion>BC V6T 1Z1</wicri:noRegion></affiliation></author><author><name sortKey="Seibert, M" sort="Seibert, M" uniqKey="Seibert M" first="M." last="Seibert">M. Seibert</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Observatories of the Carnegie Institution, 813 Santa Barbera St., Pasadena, CA 91101</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Sharp, R" sort="Sharp, R" uniqKey="Sharp R" first="R." last="Sharp">R. Sharp</name><affiliation wicri:level="1"><country xml:lang="fr">Australie</country><wicri:regionArea>Anglo‐Australian Observatory, PO Box 296, Epping, NSW 1710</wicri:regionArea><wicri:noRegion>NSW 1710</wicri:noRegion></affiliation></author><author><name sortKey="Temi, P" sort="Temi, P" uniqKey="Temi P" first="P." last="Temi">P. Temi</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Astrophysics Branch, NASA Ames Research Center, Mail Stop 2456, Moffett Field, CA 94035</wicri:regionArea><placeName><region type="state">Californie</region></placeName></affiliation></author><author><name sortKey="Tuffs, R J" sort="Tuffs, R J" uniqKey="Tuffs R" first="R. J." last="Tuffs">R. J. Tuffs</name><affiliation wicri:level="3"><country xml:lang="fr">Allemagne</country><wicri:regionArea>Max Planck Institut für Kernphysik (MPIK), Saupfercheckweg, 69117 Heidelberg</wicri:regionArea><placeName><region type="land" nuts="1">Bade-Wurtemberg</region><region type="district" nuts="2">District de Karlsruhe</region><settlement type="city">Heidelberg</settlement></placeName></affiliation></author><author><name sortKey="Van Der Werf, P" sort="Van Der Werf, P" uniqKey="Van Der Werf P" first="P." last="Van Der Werf">P. Van Der Werf</name><affiliation></affiliation><affiliation wicri:level="1"><country xml:lang="fr" wicri:curation="lc">Pays-Bas</country><wicri:regionArea>Leiden Observatory, Leiden University, PO Box 9513, NL ‐ 2300 RA Leiden</wicri:regionArea><wicri:noRegion>NL ‐ 2300 RA Leiden</wicri:noRegion></affiliation></author><author><name sortKey="Van Kampen, E" sort="Van Kampen, E" uniqKey="Van Kampen E" first="E." last="Van Kampen">E. Van Kampen</name><affiliation wicri:level="1"><country xml:lang="fr">Allemagne</country><wicri:regionArea>European Southern Observatory, Karl‐Schwarzschild‐Strasse 2, D‐85748 Garching bei München</wicri:regionArea><wicri:noRegion>85748 Garching bei München</wicri:noRegion><wicri:noRegion>D‐85748 Garching bei München</wicri:noRegion></affiliation></author></analytic><monogr></monogr><series><title level="j">Monthly Notices of the Royal Astronomical Society</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2011-09-11">2011-09-11</date><biblScope unit="volume">416</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="857">857</biblScope><biblScope unit="page" to="872">872</biblScope></imprint><idno type="ISSN">0035-8711</idno></series><idno type="istex">A0DF6586BAE8156157D7A336C1BD91E5D2E6B5C1</idno><idno type="DOI">10.1111/j.1365-2966.2011.18827.x</idno><idno type="ArticleID">MNR18827</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>methods: statistical</term><term>submillimetre: galaxies</term></keywords></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We present a technique to identify optical counterparts of 250‐μm‐selected sources from the Herschel–ATLAS survey. Of the 6621 250 μm > 32‐mJy sources in our science demonstration catalogue we find that ∼60 per cent have counterparts brighter than r = 22.4 mag in the Sloan Digital Sky Survey. Applying a likelihood ratio technique we are able to identify 2423 of the counterparts with a reliability R > 0.8. This is approximately 37 per cent of the full 250‐μm catalogue. We have estimated photometric redshifts for each of these 2423 reliable counterparts, while 1099 also have spectroscopic redshifts collated from several different sources, including the GAMA survey. We estimate the completeness of identifying counterparts as a function of redshift, and present evidence that 250‐μm‐selected Herschel–ATLAS galaxies have a bimodal redshift distribution. Those with reliable optical identifications have a redshift distribution peaking at z ≈ 0.25 ± 0.05, while submillimetre colours suggest that a significant fraction with no counterpart above the r‐band limit have z > 1. We also suggest a method for selecting populations of strongly lensed high‐redshift galaxies. Our identifications are matched to UV–NIR photometry from the GAMA survey, and these data are available as part of the Herschel–ATLAS public data release.</div></front></TEI><affiliations><list><country><li>Allemagne</li><li>Australie</li><li>Belgique</li><li>Canada</li><li>Espagne</li><li>France</li><li>Italie</li><li>Pays-Bas</li><li>États-Unis</li></country><region><li>Bade-Wurtemberg</li><li>Californie</li><li>Communauté de Madrid</li><li>District de Karlsruhe</li><li>Province de Flandre-Orientale</li><li>Région flamande</li></region><settlement><li>Gand</li><li>Heidelberg</li><li>Madrid</li></settlement><orgName><li>Université complutense de Madrid</li><li>Université de Gand</li></orgName></list><tree><noCountry><name sortKey="Baldry, I K" sort="Baldry, I K" uniqKey="Baldry I" first="I. K." last="Baldry">I. K. 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Pascale</name><name sortKey="Pohlen, M" sort="Pohlen, M" uniqKey="Pohlen M" first="M." last="Pohlen">M. Pohlen</name><name sortKey="Popescu, C C" sort="Popescu, C C" uniqKey="Popescu C" first="C. C." last="Popescu">C. C. Popescu</name><name sortKey="Prescott, M" sort="Prescott, M" uniqKey="Prescott M" first="M." last="Prescott">M. Prescott</name><name sortKey="Rigby, E E" sort="Rigby, E E" uniqKey="Rigby E" first="E. E." last="Rigby">E. E. Rigby</name><name sortKey="Robotham, A" sort="Robotham, A" uniqKey="Robotham A" first="A." last="Robotham">A. Robotham</name><name sortKey="Smith, D J B" sort="Smith, D J B" uniqKey="Smith D" first="D. J. B." last="Smith">D. J. B. Smith</name><name sortKey="Sutherland, W" sort="Sutherland, W" uniqKey="Sutherland W" first="W." last="Sutherland">W. Sutherland</name><name sortKey="Thompson, M A" sort="Thompson, M A" uniqKey="Thompson M" first="M. A." last="Thompson">M. A. 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Sharp</name></country><country name="Belgique"><region name="Région flamande"><name sortKey="Fritz, J" sort="Fritz, J" uniqKey="Fritz J" first="J." last="Fritz">J. Fritz</name></region></country><country name="Allemagne"><noRegion><name sortKey="Liske, J" sort="Liske, J" uniqKey="Liske J" first="J." last="Liske">J. Liske</name></noRegion><name sortKey="Tuffs, R J" sort="Tuffs, R J" uniqKey="Tuffs R" first="R. J." last="Tuffs">R. J. Tuffs</name><name sortKey="Van Kampen, E" sort="Van Kampen, E" uniqKey="Van Kampen E" first="E." last="Van Kampen">E. Van Kampen</name></country><country name="France"><noRegion><name sortKey="Panuzzo, P" sort="Panuzzo, P" uniqKey="Panuzzo P" first="P." last="Panuzzo">P. Panuzzo</name></noRegion></country><country name="Canada"><noRegion><name sortKey="Scott, D" sort="Scott, D" uniqKey="Scott D" first="D." last="Scott">D. Scott</name></noRegion></country><country name="Pays-Bas"><noRegion><name sortKey="Van Der Werf, P" sort="Van Der Werf, P" uniqKey="Van Der Werf P" first="P." last="Van Der Werf">P. Van Der Werf</name></noRegion></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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