The SCUBA Half Degree Extragalactic Survey – IV. Radio–mm–FIR photometric redshifts
Identifieur interne : 000210 ( Main/Exploration ); précédent : 000209; suivant : 000211The SCUBA Half Degree Extragalactic Survey – IV. Radio–mm–FIR photometric redshifts
Auteurs : Itziar Aretxaga [Mexique] ; David H. Hughes [Mexique] ; Kristen Coppin [Canada] ; Angela M. J. Mortier ; Jeff Wagg [Mexique, États-Unis] ; James S. Dunlop ; Edward L. Chapin [Canada] ; Stephen A. Eales ; Enrique Gazta Aga [Mexique, Espagne] ; Mark Halpern [Canada] ; Rob J. Ivison ; Eelco Van Kampen [Autriche] ; Douglas Scott [Canada] ; Stephen Serjeant ; Ian Smail ; Thomas Babbedge ; Andrew J. Benson [États-Unis] ; Scott Chapman [États-Unis] ; David L. Clements ; Loretta Dunne ; Simon Dye ; Duncan Farrah [États-Unis] ; Matt J. Jarvis ; Robert G. Mann ; Alexandra Pope [Canada] ; Robert Priddey ; Steve Rawlings ; Marc Seigar [États-Unis] ; Laura Silva [Italie] ; Chris Simpson ; Mattia Vaccari [Italie]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2007-08-21.
Abstract
We present the redshift distribution of the Submillimetre Common-User Bolometer Array (SCUBA) Half Degree Survey (SHADES) galaxy population based on the rest-frame radio–mm–far-infrared (FIR) colours of 120 robustly detected 850 μm sources in the Lockman Hole East (LH) and Subaru XMM–Newton Deep Field (SXDF). The redshift distribution derived from the full spectral energy distribution (SED) information is shown to be narrower than that determined from the radio–sub-mm spectral index, as more photometric bands contribute to a higher redshift accuracy. The redshift distribution of sources derived from at least two photometric bands peaks at z≈ 2.4 and has a near-Gaussian distribution, with 50 per cent (interquartile range) of sources at z= 1.8–3.1. We find a statistically significant difference between the measured redshift distributions in the two fields; the SXDF peaking at a slightly lower redshift (median z≈ 2.2) than the LH (median z≈ 2.7), which we attribute to the noise properties of the radio observations. We demonstrate, however, that there could also be field-to-field variations that are consistent with the measured differences in the redshift distributions and, hence, that the incomplete area observed by SHADES with SCUBA, despite being the largest sub-mm survey to date, may still be too small to fully characterize the bright sub-mm galaxy population. Finally, we present a brief comparison with the predicted, or assumed, redshift distributions of sub-mm galaxy formation and evolution models, and we derive the contribution of these SHADES sources and the general sub-mm galaxy population to the star formation rate density at different epochs.
Url:
DOI: 10.1111/j.1365-2966.2007.12036.x
Affiliations:
- Autriche, Canada, Espagne, Italie, Mexique, États-Unis
- Catalogne, État de New York
- Ithaca (New York)
- Université Cornell
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Radio–mm–FIR photometric redshifts</title><author><name sortKey="Aretxaga, Itziar" sort="Aretxaga, Itziar" uniqKey="Aretxaga I" first="Itziar" last="Aretxaga">Itziar Aretxaga</name><affiliation wicri:level="1"><country xml:lang="fr">Mexique</country><wicri:regionArea>Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE), Aptdo. Postal 51 y 216, 72000 Puebla, Pue.</wicri:regionArea><wicri:noRegion>Pue.</wicri:noRegion></affiliation><affiliation wicri:level="1"><country wicri:rule="url">Mexique</country></affiliation></author><author><name sortKey="Hughes, David H" sort="Hughes, David H" uniqKey="Hughes D" first="David H." last="Hughes">David H. Hughes</name><affiliation wicri:level="1"><country xml:lang="fr">Mexique</country><wicri:regionArea>Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE), Aptdo. 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Benson</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Caltech, 1200 E. California Blvd., Pasadena, CA 91125-0001</wicri:regionArea><wicri:noRegion>CA 91125-0001</wicri:noRegion></affiliation></author><author><name sortKey="Chapman, Scott" sort="Chapman, Scott" uniqKey="Chapman S" first="Scott" last="Chapman">Scott Chapman</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Caltech, 1200 E. California Blvd., Pasadena, CA 91125-0001</wicri:regionArea><wicri:noRegion>CA 91125-0001</wicri:noRegion></affiliation></author><author><name sortKey="Clements, David L" sort="Clements, David L" uniqKey="Clements D" first="David L." last="Clements">David L. Clements</name><affiliation><wicri:noCountry code="subField">2BW</wicri:noCountry></affiliation></author><author><name sortKey="Dunne, Loretta" sort="Dunne, Loretta" uniqKey="Dunne L" first="Loretta" last="Dunne">Loretta Dunne</name><affiliation><wicri:noCountry code="subField">2RD</wicri:noCountry></affiliation></author><author><name sortKey="Dye, Simon" sort="Dye, Simon" uniqKey="Dye S" first="Simon" last="Dye">Simon Dye</name><affiliation><wicri:noCountry code="subField">3YB</wicri:noCountry></affiliation></author><author><name sortKey="Farrah, Duncan" sort="Farrah, Duncan" uniqKey="Farrah D" first="Duncan" last="Farrah">Duncan Farrah</name><affiliation wicri:level="4"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Astronomy, Cornell University, Space Sciences Building, Ithaca, NY 14853</wicri:regionArea><orgName type="university">Université Cornell</orgName><placeName><settlement type="city">Ithaca (New York)</settlement><region type="state">État de New York</region></placeName></affiliation></author><author><name sortKey="Jarvis, Matt J" sort="Jarvis, Matt J" uniqKey="Jarvis M" first="Matt J." last="Jarvis">Matt J. Jarvis</name><affiliation></affiliation><affiliation><wicri:noCountry code="subField">3RH</wicri:noCountry></affiliation></author><author><name sortKey="Mann, Robert G" sort="Mann, Robert G" uniqKey="Mann R" first="Robert G." last="Mann">Robert G. Mann</name><affiliation><wicri:noCountry code="subField">3HJ</wicri:noCountry></affiliation></author><author><name sortKey="Pope, Alexandra" sort="Pope, Alexandra" uniqKey="Pope A" first="Alexandra" last="Pope">Alexandra Pope</name><affiliation wicri:level="1"><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, B.C., V6T 1Z1</wicri:regionArea><wicri:noRegion>V6T 1Z1</wicri:noRegion></affiliation></author><author><name sortKey="Priddey, Robert" sort="Priddey, Robert" uniqKey="Priddey R" first="Robert" last="Priddey">Robert Priddey</name><affiliation><wicri:noCountry code="subField">9AB</wicri:noCountry></affiliation></author><author><name sortKey="Rawlings, Steve" sort="Rawlings, Steve" uniqKey="Rawlings S" first="Steve" last="Rawlings">Steve Rawlings</name><affiliation><wicri:noCountry code="subField">3RH</wicri:noCountry></affiliation></author><author><name sortKey="Seigar, Marc" sort="Seigar, Marc" uniqKey="Seigar M" first="Marc" last="Seigar">Marc Seigar</name><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Center for Cosmology, Department of Physics & Astronomy, Univ. of California, Irvine, 4129 Frederick Reines Hall, Irvine, CA 92697-4575</wicri:regionArea><wicri:noRegion>CA 92697-4575</wicri:noRegion></affiliation></author><author><name sortKey="Silva, Laura" sort="Silva, Laura" uniqKey="Silva L" first="Laura" last="Silva">Laura Silva</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>Osservatorio Astronomico di Trieste, Via Tiepolo 11, I-341311, Trieste</wicri:regionArea><wicri:noRegion>Trieste</wicri:noRegion></affiliation></author><author><name sortKey="Simpson, Chris" sort="Simpson, Chris" uniqKey="Simpson C" first="Chris" last="Simpson">Chris Simpson</name><affiliation><wicri:noCountry code="subField">1LD</wicri:noCountry></affiliation></author><author><name sortKey="Vaccari, Mattia" sort="Vaccari, Mattia" uniqKey="Vaccari M" first="Mattia" last="Vaccari">Mattia Vaccari</name><affiliation></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>Department of Astronomy, University of Padova, Vicolo dell'Osservatorio 2, I-35122, Padova</wicri:regionArea><wicri:noRegion>Padova</wicri:noRegion></affiliation></author></analytic><monogr></monogr><series><title level="j">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbrev">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="2007-08-21">2007-08-21</date><biblScope unit="volume">379</biblScope><biblScope unit="issue">4</biblScope><biblScope unit="page" from="1571">1571</biblScope><biblScope unit="page" to="1588">1588</biblScope></imprint><idno type="ISSN">0035-8711</idno></series><idno type="istex">CD2CC11E7049EF5A1251F71F42B462D6C3ECEE90</idno><idno type="DOI">10.1111/j.1365-2966.2007.12036.x</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract">We present the redshift distribution of the Submillimetre Common-User Bolometer Array (SCUBA) Half Degree Survey (SHADES) galaxy population based on the rest-frame radio–mm–far-infrared (FIR) colours of 120 robustly detected 850 μm sources in the Lockman Hole East (LH) and Subaru XMM–Newton Deep Field (SXDF). The redshift distribution derived from the full spectral energy distribution (SED) information is shown to be narrower than that determined from the radio–sub-mm spectral index, as more photometric bands contribute to a higher redshift accuracy. The redshift distribution of sources derived from at least two photometric bands peaks at z≈ 2.4 and has a near-Gaussian distribution, with 50 per cent (interquartile range) of sources at z= 1.8–3.1. We find a statistically significant difference between the measured redshift distributions in the two fields; the SXDF peaking at a slightly lower redshift (median z≈ 2.2) than the LH (median z≈ 2.7), which we attribute to the noise properties of the radio observations. We demonstrate, however, that there could also be field-to-field variations that are consistent with the measured differences in the redshift distributions and, hence, that the incomplete area observed by SHADES with SCUBA, despite being the largest sub-mm survey to date, may still be too small to fully characterize the bright sub-mm galaxy population. Finally, we present a brief comparison with the predicted, or assumed, redshift distributions of sub-mm galaxy formation and evolution models, and we derive the contribution of these SHADES sources and the general sub-mm galaxy population to the star formation rate density at different epochs.</div></front></TEI><affiliations><list><country><li>Autriche</li><li>Canada</li><li>Espagne</li><li>Italie</li><li>Mexique</li><li>États-Unis</li></country><region><li>Catalogne</li><li>État de New York</li></region><settlement><li>Ithaca (New York)</li></settlement><orgName><li>Université Cornell</li></orgName></list><tree><noCountry><name sortKey="Babbedge, Thomas" sort="Babbedge, Thomas" uniqKey="Babbedge T" first="Thomas" last="Babbedge">Thomas Babbedge</name><name sortKey="Clements, David L" sort="Clements, David L" uniqKey="Clements D" first="David L." last="Clements">David L. Clements</name><name sortKey="Dunlop, James S" sort="Dunlop, James S" uniqKey="Dunlop J" first="James S." last="Dunlop">James S. Dunlop</name><name sortKey="Dunne, Loretta" sort="Dunne, Loretta" uniqKey="Dunne L" first="Loretta" last="Dunne">Loretta Dunne</name><name sortKey="Dye, Simon" sort="Dye, Simon" uniqKey="Dye S" first="Simon" last="Dye">Simon Dye</name><name sortKey="Eales, Stephen A" sort="Eales, Stephen A" uniqKey="Eales S" first="Stephen A." last="Eales">Stephen A. Eales</name><name sortKey="Ivison, Rob J" sort="Ivison, Rob J" uniqKey="Ivison R" first="Rob J." last="Ivison">Rob J. Ivison</name><name sortKey="Jarvis, Matt J" sort="Jarvis, Matt J" uniqKey="Jarvis M" first="Matt J." last="Jarvis">Matt J. Jarvis</name><name sortKey="Mann, Robert G" sort="Mann, Robert G" uniqKey="Mann R" first="Robert G." last="Mann">Robert G. Mann</name><name sortKey="Mortier, Angela M J" sort="Mortier, Angela M J" uniqKey="Mortier A" first="Angela M. J." last="Mortier">Angela M. J. Mortier</name><name sortKey="Priddey, Robert" sort="Priddey, Robert" uniqKey="Priddey R" first="Robert" last="Priddey">Robert Priddey</name><name sortKey="Rawlings, Steve" sort="Rawlings, Steve" uniqKey="Rawlings S" first="Steve" last="Rawlings">Steve Rawlings</name><name sortKey="Serjeant, Stephen" sort="Serjeant, Stephen" uniqKey="Serjeant S" first="Stephen" last="Serjeant">Stephen Serjeant</name><name sortKey="Simpson, Chris" sort="Simpson, Chris" uniqKey="Simpson C" first="Chris" last="Simpson">Chris Simpson</name><name sortKey="Smail, Ian" sort="Smail, Ian" uniqKey="Smail I" first="Ian" last="Smail">Ian Smail</name></noCountry><country name="Mexique"><noRegion><name sortKey="Aretxaga, Itziar" sort="Aretxaga, Itziar" uniqKey="Aretxaga I" first="Itziar" last="Aretxaga">Itziar Aretxaga</name></noRegion><name sortKey="Aretxaga, Itziar" sort="Aretxaga, Itziar" uniqKey="Aretxaga I" first="Itziar" last="Aretxaga">Itziar Aretxaga</name><name sortKey="Gazta Aga, Enrique" sort="Gazta Aga, Enrique" uniqKey="Gazta Aga E" first="Enrique" last="Gazta Aga">Enrique Gazta Aga</name><name sortKey="Hughes, David H" sort="Hughes, David H" uniqKey="Hughes D" first="David H." last="Hughes">David H. Hughes</name><name sortKey="Wagg, Jeff" sort="Wagg, Jeff" uniqKey="Wagg J" first="Jeff" last="Wagg">Jeff Wagg</name></country><country name="Canada"><noRegion><name sortKey="Coppin, Kristen" sort="Coppin, Kristen" uniqKey="Coppin K" first="Kristen" last="Coppin">Kristen Coppin</name></noRegion><name sortKey="Chapin, Edward L" sort="Chapin, Edward L" uniqKey="Chapin E" first="Edward L." last="Chapin">Edward L. Chapin</name><name sortKey="Halpern, Mark" sort="Halpern, Mark" uniqKey="Halpern M" first="Mark" last="Halpern">Mark Halpern</name><name sortKey="Pope, Alexandra" sort="Pope, Alexandra" uniqKey="Pope A" first="Alexandra" last="Pope">Alexandra Pope</name><name sortKey="Scott, Douglas" sort="Scott, Douglas" uniqKey="Scott D" first="Douglas" last="Scott">Douglas Scott</name></country><country name="États-Unis"><noRegion><name sortKey="Wagg, Jeff" sort="Wagg, Jeff" uniqKey="Wagg J" first="Jeff" last="Wagg">Jeff Wagg</name></noRegion><name sortKey="Benson, Andrew J" sort="Benson, Andrew J" uniqKey="Benson A" first="Andrew J." last="Benson">Andrew J. Benson</name><name sortKey="Chapman, Scott" sort="Chapman, Scott" uniqKey="Chapman S" first="Scott" last="Chapman">Scott Chapman</name><name sortKey="Farrah, Duncan" sort="Farrah, Duncan" uniqKey="Farrah D" first="Duncan" last="Farrah">Duncan Farrah</name><name sortKey="Seigar, Marc" sort="Seigar, Marc" uniqKey="Seigar M" first="Marc" last="Seigar">Marc Seigar</name></country><country name="Espagne"><region name="Catalogne"><name sortKey="Gazta Aga, Enrique" sort="Gazta Aga, Enrique" uniqKey="Gazta Aga E" first="Enrique" last="Gazta Aga">Enrique Gazta Aga</name></region></country><country name="Autriche"><noRegion><name sortKey="Van Kampen, Eelco" sort="Van Kampen, Eelco" uniqKey="Van Kampen E" first="Eelco" last="Van Kampen">Eelco Van Kampen</name></noRegion></country><country name="Italie"><noRegion><name sortKey="Silva, Laura" sort="Silva, Laura" uniqKey="Silva L" first="Laura" last="Silva">Laura Silva</name></noRegion><name sortKey="Vaccari, Mattia" sort="Vaccari, Mattia" uniqKey="Vaccari M" first="Mattia" last="Vaccari">Mattia Vaccari</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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|area= CaltechV1
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|étape= Exploration
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|clé= ISTEX:CD2CC11E7049EF5A1251F71F42B462D6C3ECEE90
|texte= The SCUBA Half Degree Extragalactic Survey – IV. Radio–mm–FIR photometric redshifts
}}
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