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<ri:Resource created="2011-09-27T12:00:06Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>86 Herschel sources SED model parameters</title><shortName>J/MNRAS/409/2</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/409/2</identifier><altIdentifier>doi:10.26093/cds/vizier.74090002</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rowan-Robinson M.</name></creator><creator><name>Roseboom I.G.</name></creator><creator><name>Vaccari M.</name></creator><creator><name>Amblard A.</name></creator><creator><name>Arumugam V.,Auld R.</name></creator><creator><name>Aussel H.</name></creator><creator><name>Babbedge T.</name></creator><creator><name>Blain A.</name></creator><creator><name>Bock J.</name></creator><creator><name>Boselli A.</name></creator><creator><name>Brisbin D.,Buat V.</name></creator><creator><name>Burgarella D.</name></creator><creator><name>Castro-Rodriguez N.</name></creator><creator><name>Cava A.</name></creator><creator><name>Chanial P.,Clements D.L.</name></creator><creator><name>Conley A.</name></creator><creator><name>Conversi L.</name></creator><creator><name>Cooray A.</name></creator><creator><name>Dowell C.D.</name></creator><creator><name>Dwek E.,Dye S.</name></creator><creator><name>Eales S.</name></creator><creator><name>Elbaz D.</name></creator><creator><name>Farrah D.</name></creator><creator><name>Fox M.</name></creator><creator><name>Franceschini A.</name></creator><creator><name>Gear W.,Glenn J.</name></creator><creator><name>Gonzalez Solares E.A.</name></creator><creator><name>Griffin M.</name></creator><creator><name>Halpern M.</name></creator><creator><name>Hatziminaoglou E.,Huang J.</name></creator><creator><name>Ibar E.</name></creator><creator><name>Isaak K.</name></creator><creator><name>Ivison R.J.</name></creator><creator><name>Lagache G.</name></creator><creator><name>Levenson L.</name></creator><creator><name>Lu N.,Madden S.</name></creator><creator><name>Maffei B.</name></creator><creator><name>Mainetti G.</name></creator><creator><name>Marchetti L.</name></creator><creator><name>Mortier A.M.J.,Nguyen H.T.</name></creator><creator><name>O'halloran B.</name></creator><creator><name>Oliver S.J.</name></creator><creator><name>Omont A.</name></creator><creator><name>Page M.J.</name></creator><creator><name>Panuzzo P.,Papageorgiou A.</name></creator><creator><name>Patel H.</name></creator><creator><name>Pearson C.P.</name></creator><creator><name>Perez Fournon I.</name></creator><creator><name>Pohlen M.,Rawlings J.I.</name></creator><creator><name>Raymond G.</name></creator><creator><name>Rigopoulou D.</name></creator><creator><name>Rizzo D.</name></creator><creator><name>Schulz B.</name></creator><creator><name>Scott D.,Seymour N.</name></creator><creator><name>Shupe D.L.</name></creator><creator><name>Smith A.J.</name></creator><creator><name>Stevens J.A.</name></creator><creator><name>Symeonidis M.,Trichas M.</name></creator><creator><name>Tugwell K.E.</name></creator><creator><name>Valtchanov I.</name></creator><creator><name>Vigroux L.</name></creator><creator><name>Wang L.</name></creator><creator><name>Ward R.,Wright G.</name></creator><creator><name>Xu C.K.</name></creator><creator><name>Zemcov M.</name></creator><date role="Updated">2024-07-12T20:14:55Z</date><date role="Created">2011-09-27T12:00:06Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>infrared-sources</subject><subject>redshifted</subject><subject>spectral-energy-distribution</subject><description>We present spectral energy distributions (SEDs) for 86 Herschel sources detected at 5{sigma} at 250, 350 and 500um in the HerMES SWIRE-Lockman field. We explore whether existing models for starbursts, quiescent star-forming galaxies and active galactic nucleus dust tori are able to model the full range of SEDs measured with Herschel. We find that while many galaxies (~56 per cent) are well fitted with the templates used to fit IRAS, Infrared Space Observatory (ISO) and Spitzer sources, for about half the galaxies two new templates are required: quiescent ('cirrus') models with colder (10-20K) dust and a young starburst model with higher optical depth than Arp 220. Predictions of submillimetre fluxes based on model fits to 4.5-24um data agree rather poorly with the observed fluxes, but the agreement is better for fits to 4.5-70um data. Herschel galaxies detected at 500um tend to be those with the highest dust masses.</description><source format="bibcode">2010MNRAS.409....2R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/409/2</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/290">II/290 : SWIRE Photometric Redshift Catalogue (Rowan-Robinson+, 2008)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/409/2</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/409/2</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/409/2</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/409/2</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/409/2</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/409/2</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/409/2/table2 (*Parameters for SED models, complete sample of 86 three-band sources)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/409/2/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/409/2/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/409/2/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>162.9482</ra><dec>58.26883</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/1519 6/6069-6071 6073 6090 6112 6114 7444</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/409/2?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/409/2/table2</name><description>*Parameters for SED models, complete sample of 86 three-band sources</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Code</name><description>[YZ] Y = Young starburst; Z = z&gt;3</description><ucd>meta.id;stat.fit</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_z</name><description>[)] ) for photometric redshift</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logLc5</name><description>? 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