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<ri:Resource created="2023-11-09T09:32:49Z" 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>Resolved molecular gas in nearby galaxies</title><shortName>J/MNRAS/500/1261</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/500/1261</identifier><altIdentifier>doi:10.26093/cds/vizier.75001261</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chown R.</name></creator><creator><name>Li C.</name></creator><creator><name>Parker L.</name></creator><creator><name>Wilson C.D.</name></creator><creator><name>Li N.</name></creator><creator><name>Gao Y.</name></creator><date role="Updated">2024-08-21T20:16:42Z</date><date role="Created">2023-11-09T09:32:49Z</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>chemically-peculiar-stars</subject><subject>extinction</subject><subject>star-forming-regions</subject><subject>infrared-astronomy</subject><subject>visible-astronomy</subject><subject>radio-astronomy</subject><description>A relationship between dust-reprocessed light from recent star formation and the amount of star-forming gas in a galaxy produces a correlation between Wide-field Infrared Survey Explorer (WISE) 12{mu}m emission and CO line emission. Here, we explore this correlation on kiloparsec scales with CO(1-0) maps from EDGE-CALIFA matched in resolution to WISE 12{mu}m images. We find strong CO-12{mu}m correlations within each galaxy and we show that the scatter in the global CO-12{mu}m correlation is largely driven by differences from galaxy to galaxy. The correlation is stronger than that between star formation rate and H_2_ surface densities [{Sigma}(H_2_)]. We explore multivariable regression to predict {Sigma}(H_2_) in star-forming pixels using the WISE 12{mu}m data combined with global and resolved galaxy properties, and provide the fit parameters for the best estimators. We find that {Sigma}(H_2_) estimators that include {Sigma}(12{mu}m) are able to predict {Sigma}(H_2_) more accurately than estimators that include resolved optical properties instead of {Sigma}(12{mu}m). These results suggest that 12{mu}m emission and H_2_ as traced by CO emission are physically connected at kiloparsec scales. This may be due to a connection between polycyclic aromatic hydrocarbon emission and the presence of H_2_. The best single-property estimator is log({Sigma}(H_2_)/M_{sun}_pc^-2^)= (0.48+/-0.01)+(0.71+/-0.01)log({Sigma}(12{mu}m)/L_{sun}_pc^-2^). This correlation can be used to efficiently estimate {Sigma}(H_2_) down to at least 1M_{sun}_pc^-2^ in star-forming regions within nearby galaxies.</description><source format="bibcode">2021MNRAS.500.1261C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/500/1261</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/J/ApJ/846/159">J/ApJ/846/159 : Interferometric CO obs. of 126 CALIFA galaxies</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/500/1261</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/500/1261</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/500/1261</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/500/1261</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/500/1261</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/500/1261</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/500/1261/global (Global properties of the galaxies in our sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/500/1261/global?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/500/1261/global?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/500/1261/global?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>233.7387</ra><dec>23.5029</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/975 2229 2254 2273-2274 2290 2641 4167 4178 4342 4445 4507 4511 4813 4840 4843 4950 4993 5332 5593 6214 6240 6261 6270 6342 6977 7214 7309 7340 7591 7824 7834 8480 8492 8498 8552 8563 8646 8673 8743 9124 9187 9216 9220 9381 9622 9628 9718 9875 9882-9883 9885 9974 10025 10200 10213 10280 10380-10381 10515 10566 10583 10588 10612 10628-10629 10705 10739-10740 10752 10778 10846 10987 11070 11164 11196 11290 11372 11374 11832 11944 18779 20417 26495 28322 28458 28491 28617 31642 31689 31736 32462</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/500/1261?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/500/1261/global</name><description>Global properties of the galaxies in our sample</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType><flag>nullable</flag></column><column><name>Name</name><description>Galaxy name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><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>logSFUV</name><description>? Logarithm of the far-UV surface density {Sigma}_FUV_</description><unit>log(1e+35W.kpc**-2)</unit><ucd>phot.flux.density.sb</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Nx</name><description>Number of pixels in the x-direction</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logSNUV</name><description>? Logarithm of the near-UV surface density {Sigma}_NUV_</description><unit>log(1e+35W.kpc**-2)</unit><ucd>phot.flux.density.sb</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logSW4</name><description>? Logarithm of the WISE W4 (22{mu}m) surface density {Sigma}_W4_</description><unit>log(1e+35W.kpc**-2)</unit><ucd>phot.flux.density.sb</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logSM*</name><description>Logarithm of the stellar mass surface density {Sigma}_M*_</description><unit>log(solMass.kpc**-2)</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AV</name><description>? Extinction measured from the Balmer decrement</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b/a</name><description>? Minor-to-major axial ratio from CALIFA synthetic photometry</description><ucd>phys.angSize;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B/T</name><description>? Bulge-to-total ratio from g-band photometry</description><ucd>phot.mag.sb;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>12+logO/H</name><description>? Gas phase metallicity</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n</name><description>? Sersic index from g-band photometry</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u-r</name><description>Colour from CALIFA synthetic photometry (SDSS filters applied to extinction-corrected spectra)</description><unit>mag</unit><ucd>phot.color;em.opt.U;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logsigma</name><description>? Logarithm of the bulge velocity dispersion</description><unit>log(km.s**-1)</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logcosi</name><description>Logarithm of the cosine of the inclination</description><ucd>phys.size.axisRatio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logSTIR</name><description>? Logarithm of the total-IR (8-1000{mu}m) surface density {Sigma}_TIR_</description><unit>log(1e+35W.kpc**-2)</unit><ucd>phot.flux.density.sb</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logDMpc</name><description>Logarithm of the luminosity distance from Bolatto et al. (2017ApJ...846..159B, Cat. 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Logarithm of the stellar mass surface density {Sigma}_M*_</description><unit>log(solMass.pc**-2)</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logSSFR</name><description>? Logarithm of the star formation rate surface density {Sigma}_SFR_</description><unit>log(solMass.yr**-1.kpc**-2)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logSSFR</name><description>? Error on logSSFR</description><unit>log(solMass.yr**-1.kpc**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AV</name><description>? Extinction measured from the Balmer decrement</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logLCO</name><description>[]? Error on logLCO</description><unit>log(K.pc**2.km.s**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logLCOsim</name><description>? Logarithm of the CO luminosity using the Simple method, including all pixels</description><unit>log(K.pc**2.km.s**-1)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logLCOsim</name><description>[]? Error on logLCOsim</description><unit>log(K.pc**2.km.s**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logSH2</name><description>? 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