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<ri:Resource created="2019-08-13T09:03:16Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>[ESS2003] Q2343-BX610 reduced PdBI spectra</title><shortName>J/A+A/628/A104</shortName><identifier>ivo://CDS.VizieR/J/A+A/628/A104</identifier><altIdentifier>doi:10.26093/cds/vizier.36280104</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brisbin D.</name></creator><creator><name>Aravena M.</name></creator><creator><name>Daddi E.</name></creator><creator><name>Dannerbauer H.</name></creator><creator><name>Decarli R.,Gonzalez Lopez J.</name></creator><creator><name>Riechers D.</name></creator><creator><name>Wagg J.</name></creator><date role="Updated">2019-08-21T11:46:26Z</date><date role="Created">2019-08-13T09:03:16Z</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>spectroscopy</subject><subject>radio-spectroscopy</subject><description>We have used the Plateau De Bure Interferometer to observe multiple CO and neutral carbon transitions in a z=2.2 main sequence disk galaxy, BX610. Our observation of CO(7-6), CO(4-3) and both far infrared [CI] lines complements previous observations of H-alpha and low-J CO, and reveal a galaxy that is vigorously forming stars with UV fields, (Log(G/G_0_)&lt;3.25), less extreme than local ULIRGs or most starbursting submillimeter galaxies in the early universe. Our observations allow new independent estimates of the cold gas mass which indicate M_gas_~2x10^11^M_{sun}_, and suggest a modestly larger alpha_CO value of ~8.2. The corresponding gas depletion timescale is ~1.5Gyr. In addition to gas of modest density (Log(n[cm^-3^])&lt;3) heated by star formation, BX610 shows evidence for a significant second gas component responsible for the strong high-J CO emission. This second component might either be a high density molecular gas component heated by star formation in a typical photodissociation region, or it could be molecular gas excited by low velocity C shocks. The CO(7-6) to far infrared luminosity ratio we observe is significantly higher than typical star forming galaxies and suggests that CO(7-6) is not a reliable star formation tracer in this galaxy.</description><source format="bibcode">2019A&amp;A...628A.104B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/628/A104</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/A+A/628/A104</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/628/A104</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/628/A104</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/628/A104</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/628/A104</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/628/A104</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Millimeter</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/628/A104/co43</name><description>CO(4-3) spectrum</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>Freq</name><description>Observed frequency</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fdens</name><description>Flux density</description><unit>mJy/beam</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/628/A104/ci10</name><description>[CI](1-0) spectrum</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>Freq</name><description>Observed frequency</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fdens</name><description>Flux density</description><unit>mJy/beam</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/628/A104/250ghz</name><description>Spectrum covering the CO(7-6) and [CI](2-1) emission lines</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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