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The SCUBA Half‐Degree Extragalactic Survey (SHADES) – VIII. The nature of faint submillimetre galaxies in SHADES, SWIRE and SXDF surveys

Identifieur interne : 000178 ( Main/Exploration ); précédent : 000177; suivant : 000179

The SCUBA Half‐Degree Extragalactic Survey (SHADES) – VIII. The nature of faint submillimetre galaxies in SHADES, SWIRE and SXDF surveys

Auteurs : D. L. Clements [Royaume-Uni] ; M. Vaccari ; T. Babbedge ; S. Oliver ; M. Rowan-Robinson ; P. Davoodi ; R. Ivison ; D. Farrah [États-Unis] ; J. Dunlop ; Dave Shupe [États-Unis] ; I. Waddington ; C. Simpson ; H. Furusawa [États-Unis] ; S. Serjeant ; A. Afonso-Luis [Espagne] ; D. M. Alexander ; I. Aretxaga [Mexique] ; A. Blain [États-Unis] ; C. Borys [États-Unis] ; S. Chapman [États-Unis] ; K. Coppin ; L. Dunne ; S. Dye ; S. A. Eales ; T. Evans [États-Unis] ; F. Fang [États-Unis] ; D. Frayer [États-Unis] ; M. Fox ; W. K. Gear ; T. R. Greve [États-Unis] ; M. Halpern [Canada] ; D. H. Hughes [Mexique] ; T. Jenness [États-Unis] ; C. J. Lonsdale [États-Unis] ; A. M. J. Mortier ; M. J. Page ; A. Pope [Canada] ; R. S. Priddey ; S. Rawlings ; R. S. Savage ; D. Scott [Canada] ; S. E. Scott ; K. Sekiguchi [États-Unis, Japon] ; I. Smail ; H. E. Smith [États-Unis] ; J. A. Stevens ; J. Surace [États-Unis] ; T. Takagi [Japon] ; E. Van Kampen [Autriche]

Source :

RBID : ISTEX:2385F61927C77DB27CD3B8795B154DC4C8F24908

English descriptors

Abstract

We present the optical‐to‐submillimetre spectral energy distributions (SEDs) for 33 radio and mid‐infrared (mid‐IR) identified submillimetre galaxies discovered via the SHADES 850‐μm SCUBA imaging in the Subaru‐XMM Deep Field (SXDF). Optical data for the sources come from the SXDF and mid‐ and far‐IR fluxes from SWIRE. We obtain photometric redshift estimates for our sources using optical and IRAC 3.6‐ and 4.5‐μm fluxes. We then fit SED templates to the longer wavelength data to determine the nature of the far‐IR emission that dominates the bolometric luminosity of these sources. The IR template fits are also used to resolve ambiguous identifications and cases of redshift aliasing. The redshift distribution obtained broadly matches previous results for submillimetre sources and on the SHADES SXDF field. Our template fitting finds that active galactic nuclei, while present in about 10 per cent of our sources, do not contribute significantly to their bolometric luminosity. Dust heating by starbursts, with either Arp220 or M82 type SEDs, appears to be responsible for the luminosity in most sources (23/33 are fitted by Arp220 templates, 2/33 by the warmer M82 templates). 8/33 sources, in contrast, are fitted by a cooler cirrus dust template, suggesting that cold dust has a role in some of these highly luminous objects. Three of our sources appear to have multiple identifications or components at the same redshift, but we find no statistical evidence that close associations are common among our SHADES sources. Examination of rest‐frame K‐band luminosity suggests that ‘downsizing’ is underway in the submillimetre galaxy population, with lower redshift systems lying in lower mass host galaxies. Of our 33 identifications six are found to be of lower reliability but their exclusion would not significantly alter our conclusions.

Url:
DOI: 10.1111/j.1365-2966.2008.13172.x


Affiliations:


Links toward previous steps (curation, corpus...)


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<wicri:regionArea>Center for Astrophysics and Space Sciences, University of California San Diego, La Jolla, CA 92063‐0424</wicri:regionArea>
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<country xml:lang="fr">Canada</country>
<wicri:regionArea>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1</wicri:regionArea>
<wicri:noRegion>BC V6T 1Z1</wicri:noRegion>
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<name sortKey="Priddey, R S" sort="Priddey, R S" uniqKey="Priddey R" first="R. S." last="Priddey">R. S. Priddey</name>
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<name sortKey="Scott, D" sort="Scott, D" uniqKey="Scott D" first="D." last="Scott">D. Scott</name>
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<country xml:lang="fr">Canada</country>
<wicri:regionArea>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1</wicri:regionArea>
<wicri:noRegion>BC V6T 1Z1</wicri:noRegion>
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<name sortKey="Scott, S E" sort="Scott, S E" uniqKey="Scott S" first="S. E." last="Scott">S. E. Scott</name>
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<name sortKey="Sekiguchi, K" sort="Sekiguchi, K" uniqKey="Sekiguchi K" first="K." last="Sekiguchi">K. Sekiguchi</name>
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<country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Subaru Telescope, National Optical Astronomy Observatory of Japan, 650 N A'ohoku Place, Hilo, HI 96720</wicri:regionArea>
<wicri:noRegion>HI 96720</wicri:noRegion>
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<wicri:regionArea>National Astronomical Observatory of Japan, Mitaka, Tokyo 181‐8588</wicri:regionArea>
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<region type="région">Région de Kantō</region>
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<name sortKey="Smail, I" sort="Smail, I" uniqKey="Smail I" first="I." last="Smail">I. Smail</name>
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<name sortKey="Smith, H E" sort="Smith, H E" uniqKey="Smith H" first="H. E." last="Smith">H. E. Smith</name>
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<country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Center for Astrophysics and Space Sciences, University of California San Diego, La Jolla, CA 92063‐0424</wicri:regionArea>
<wicri:noRegion>CA 92063‐0424</wicri:noRegion>
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</author>
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<name sortKey="Stevens, J A" sort="Stevens, J A" uniqKey="Stevens J" first="J. A." last="Stevens">J. A. Stevens</name>
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<name sortKey="Surace, J" sort="Surace, J" uniqKey="Surace J" first="J." last="Surace">J. Surace</name>
<affiliation wicri:level="1">
<country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Spitzer Science Center, MS 220‐6, Caltech, Jet Propulsion Lab, Pasadena, CA 91125</wicri:regionArea>
<wicri:noRegion>CA 91125</wicri:noRegion>
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<author>
<name sortKey="Takagi, T" sort="Takagi, T" uniqKey="Takagi T" first="T." last="Takagi">T. Takagi</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Japon</country>
<wicri:regionArea>Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa 229‐8510</wicri:regionArea>
<wicri:noRegion>Kanagawa 229‐8510</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">Autriche</country>
<wicri:regionArea>Institute for Astro‐ and Particle Physics, University of Innsbruck, Technikerstr. 25, A‐6020 Innsbruck</wicri:regionArea>
<wicri:noRegion>A‐6020 Innsbruck</wicri:noRegion>
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<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="2008-06-11">2008-06-11</date>
<biblScope unit="volume">387</biblScope>
<biblScope unit="issue">1</biblScope>
<biblScope unit="page" from="247">247</biblScope>
<biblScope unit="page" to="267">267</biblScope>
</imprint>
<idno type="ISSN">0035-8711</idno>
</series>
<idno type="istex">2385F61927C77DB27CD3B8795B154DC4C8F24908</idno>
<idno type="DOI">10.1111/j.1365-2966.2008.13172.x</idno>
<idno type="ArticleID">MNR13172</idno>
</biblStruct>
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<idno type="ISSN">0035-8711</idno>
</seriesStmt>
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<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>galaxies: high‐redshift</term>
<term>infrared: galaxies</term>
<term>submillimetre</term>
</keywords>
</textClass>
<langUsage>
<language ident="en">en</language>
</langUsage>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">We present the optical‐to‐submillimetre spectral energy distributions (SEDs) for 33 radio and mid‐infrared (mid‐IR) identified submillimetre galaxies discovered via the SHADES 850‐μm SCUBA imaging in the Subaru‐XMM Deep Field (SXDF). Optical data for the sources come from the SXDF and mid‐ and far‐IR fluxes from SWIRE. We obtain photometric redshift estimates for our sources using optical and IRAC 3.6‐ and 4.5‐μm fluxes. We then fit SED templates to the longer wavelength data to determine the nature of the far‐IR emission that dominates the bolometric luminosity of these sources. The IR template fits are also used to resolve ambiguous identifications and cases of redshift aliasing. The redshift distribution obtained broadly matches previous results for submillimetre sources and on the SHADES SXDF field. Our template fitting finds that active galactic nuclei, while present in about 10 per cent of our sources, do not contribute significantly to their bolometric luminosity. Dust heating by starbursts, with either Arp220 or M82 type SEDs, appears to be responsible for the luminosity in most sources (23/33 are fitted by Arp220 templates, 2/33 by the warmer M82 templates). 8/33 sources, in contrast, are fitted by a cooler cirrus dust template, suggesting that cold dust has a role in some of these highly luminous objects. Three of our sources appear to have multiple identifications or components at the same redshift, but we find no statistical evidence that close associations are common among our SHADES sources. Examination of rest‐frame K‐band luminosity suggests that ‘downsizing’ is underway in the submillimetre galaxy population, with lower redshift systems lying in lower mass host galaxies. Of our 33 identifications six are found to be of lower reliability but their exclusion would not significantly alter our conclusions.</div>
</front>
</TEI>
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<list>
<country>
<li>Autriche</li>
<li>Canada</li>
<li>Espagne</li>
<li>Japon</li>
<li>Mexique</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region>
<li>Région de Kantō</li>
<li>État de New York</li>
</region>
<settlement>
<li>Ithaca (New York)</li>
<li>Tokyo</li>
</settlement>
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<li>Université Cornell</li>
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<name sortKey="Coppin, K" sort="Coppin, K" uniqKey="Coppin K" first="K." last="Coppin">K. Coppin</name>
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<name sortKey="Dunne, L" sort="Dunne, L" uniqKey="Dunne L" first="L." last="Dunne">L. Dunne</name>
<name sortKey="Dye, S" sort="Dye, S" uniqKey="Dye S" first="S." last="Dye">S. Dye</name>
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<name sortKey="Fox, M" sort="Fox, M" uniqKey="Fox M" first="M." last="Fox">M. Fox</name>
<name sortKey="Gear, W K" sort="Gear, W K" uniqKey="Gear W" first="W. K." last="Gear">W. K. Gear</name>
<name sortKey="Ivison, R" sort="Ivison, R" uniqKey="Ivison R" first="R." last="Ivison">R. Ivison</name>
<name sortKey="Mortier, A M J" sort="Mortier, A M J" uniqKey="Mortier A" first="A. M. J." last="Mortier">A. M. J. Mortier</name>
<name sortKey="Oliver, S" sort="Oliver, S" uniqKey="Oliver S" first="S." last="Oliver">S. Oliver</name>
<name sortKey="Page, M J" sort="Page, M J" uniqKey="Page M" first="M. J." last="Page">M. J. Page</name>
<name sortKey="Priddey, R S" sort="Priddey, R S" uniqKey="Priddey R" first="R. S." last="Priddey">R. S. Priddey</name>
<name sortKey="Rawlings, S" sort="Rawlings, S" uniqKey="Rawlings S" first="S." last="Rawlings">S. Rawlings</name>
<name sortKey="Rowan Obinson, M" sort="Rowan Obinson, M" uniqKey="Rowan Obinson M" first="M." last="Rowan-Robinson">M. Rowan-Robinson</name>
<name sortKey="Savage, R S" sort="Savage, R S" uniqKey="Savage R" first="R. S." last="Savage">R. S. Savage</name>
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<name sortKey="Simpson, C" sort="Simpson, C" uniqKey="Simpson C" first="C." last="Simpson">C. Simpson</name>
<name sortKey="Smail, I" sort="Smail, I" uniqKey="Smail I" first="I." last="Smail">I. Smail</name>
<name sortKey="Stevens, J A" sort="Stevens, J A" uniqKey="Stevens J" first="J. A." last="Stevens">J. A. Stevens</name>
<name sortKey="Vaccari, M" sort="Vaccari, M" uniqKey="Vaccari M" first="M." last="Vaccari">M. Vaccari</name>
<name sortKey="Waddington, I" sort="Waddington, I" uniqKey="Waddington I" first="I." last="Waddington">I. Waddington</name>
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<name sortKey="Clements, D L" sort="Clements, D L" uniqKey="Clements D" first="D. L." last="Clements">D. L. Clements</name>
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<region name="État de New York">
<name sortKey="Farrah, D" sort="Farrah, D" uniqKey="Farrah D" first="D." last="Farrah">D. Farrah</name>
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<name sortKey="Blain, A" sort="Blain, A" uniqKey="Blain A" first="A." last="Blain">A. Blain</name>
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<name sortKey="Chapman, S" sort="Chapman, S" uniqKey="Chapman S" first="S." last="Chapman">S. Chapman</name>
<name sortKey="Evans, T" sort="Evans, T" uniqKey="Evans T" first="T." last="Evans">T. Evans</name>
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<name sortKey="Lonsdale, C J" sort="Lonsdale, C J" uniqKey="Lonsdale C" first="C. J." last="Lonsdale">C. J. Lonsdale</name>
<name sortKey="Lonsdale, C J" sort="Lonsdale, C J" uniqKey="Lonsdale C" first="C. J." last="Lonsdale">C. J. Lonsdale</name>
<name sortKey="Sekiguchi, K" sort="Sekiguchi, K" uniqKey="Sekiguchi K" first="K." last="Sekiguchi">K. Sekiguchi</name>
<name sortKey="Shupe, Dave" sort="Shupe, Dave" uniqKey="Shupe D" first="Dave" last="Shupe">Dave Shupe</name>
<name sortKey="Smith, H E" sort="Smith, H E" uniqKey="Smith H" first="H. E." last="Smith">H. E. Smith</name>
<name sortKey="Surace, J" sort="Surace, J" uniqKey="Surace J" first="J." last="Surace">J. Surace</name>
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<name sortKey="Afonso Uis, A" sort="Afonso Uis, A" uniqKey="Afonso Uis A" first="A." last="Afonso-Luis">A. Afonso-Luis</name>
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<name sortKey="Hughes, D H" sort="Hughes, D H" uniqKey="Hughes D" first="D. H." last="Hughes">D. H. Hughes</name>
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<name sortKey="Halpern, M" sort="Halpern, M" uniqKey="Halpern M" first="M." last="Halpern">M. Halpern</name>
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<name sortKey="Pope, A" sort="Pope, A" uniqKey="Pope A" first="A." last="Pope">A. Pope</name>
<name sortKey="Scott, D" sort="Scott, D" uniqKey="Scott D" first="D." last="Scott">D. Scott</name>
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<region name="Région de Kantō">
<name sortKey="Sekiguchi, K" sort="Sekiguchi, K" uniqKey="Sekiguchi K" first="K." last="Sekiguchi">K. Sekiguchi</name>
</region>
<name sortKey="Takagi, T" sort="Takagi, T" uniqKey="Takagi T" first="T." last="Takagi">T. Takagi</name>
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<name sortKey="Van Kampen, E" sort="Van Kampen, E" uniqKey="Van Kampen E" first="E." last="Van Kampen">E. Van Kampen</name>
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