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<ri:Resource created="2013-06-21T15:33:21Z" 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>UV/far-IR data of infrared excess sources</title><shortName>J/MNRAS/406/420</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/406/420</identifier><altIdentifier>doi:10.26093/cds/vizier.74060420</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Georgakakis A.</name></creator><creator><name>Rowan-Robinson M.</name></creator><creator><name>Nandra K.</name></creator><creator><name>Digby-North J.,Perez-Gonzalez P.G.</name></creator><creator><name>Barro G.</name></creator><date role="Updated">2024-07-12T20:14:22Z</date><date role="Created">2013-06-21T15:33:21Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We explore the nature of Infrared Excess sources (IRX), which are proposed as candidates for luminous [LX(2-10keV)&gt;10^43^erg/s] Compton thick (NH&gt;2x10^24^cm^-2^) QSOs at z~~2. Lower redshift, z~~1, analogues of the distant IRX population are identified by first redshifting to z=2 the spectral energy distributions (SEDs) of all sources with secure spectroscopic redshifts in the AEGIS (6488) and the GOODS-North (1784) surveys and then selecting those that qualify as IRX sources at that redshift. A total of 19 galaxies are selected. The mean redshift of the sample is z~~1. We do not find strong evidence for Compton thick QSOs in the sample. For nine sources with X-ray counterparts, the X-ray spectra are consistent with Compton thin active galactic nucleus (AGN). Only three of them show tentative evidence for Compton thick obscuration. The SEDs of the X-ray undetected population are consistent with starburst activity.</description><source format="bibcode">2010MNRAS.406..420G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/406/420</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/301">II/301 : The DEEP2-DR1 Photometric Catalog (Coil+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/658/1264">J/ApJ/658/1264 : IR-excess sources in GLIMPSE and MSX (Uzpen+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/180/102">J/ApJS/180/102 : AEGIS-X: Chandra deep survey (Laird+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/634/128">J/ApJ/634/128 : 16{mu}m imaging around the HDF-N (Teplitz+, 2005)</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/406/420</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/406/420</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/406/420</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/406/420</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/406/420</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/406/420</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/406/420/sample (The sample: physical parameters and X-ray properties)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/406/420/sample?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/406/420/sample?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/406/420/sample?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>214.072375</ra><dec>52.210625</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/11252 11424-11425 11428</spatial><spectral>2.4016587514425055e-21 5.950631229554308e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/406/420?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/406/420/sample</name><description>The sample: physical parameters and X-ray properties</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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DEEP2 R-band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logR</name><description>? rms uncertainty on logR</description><unit>log(uJy)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logI</name><description>DEEP2 I-band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logI</name><description>rms uncertainty on logI</description><unit>log(uJy)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logz</name><description>? CFHT/Megacam z-band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logz</name><description>? rms uncertainty on logz</description><unit>log(uJy)</unit><ucd>stat.error;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log3.6</name><description>Spitzer/IRAC 3.6um band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log3.6</name><description>rms uncertainty on log3.6</description><unit>log(uJy)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log4.5</name><description>Spitzer/IRAC 4.5um band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log4.5</name><description>rms uncertainty on log4.5</description><unit>log(uJy)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log5.8</name><description>Spitzer/IRAC 5.8um band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log5.8</name><description>rms uncertainty on log5.8</description><unit>log(uJy)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log8.0</name><description>? Spitzer/IRAC 8.0um band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log8.0</name><description>? rms uncertainty on log8.0</description><unit>log(uJy)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log24</name><description>? Spitzer/MIPS 24um band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log24</name><description>? rms uncertainty on log24</description><unit>log(uJy)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log70</name><description>? Spitzer/MIPS 70um band flux density</description><unit>log(uJy)</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log70</name><description>? rms uncertainty on log70</description><unit>log(uJy)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>