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<ri:Resource created="2018-09-07T07:55:59Z" 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>Probing star formation and ISM properties. II</title><shortName>J/A+A/616/A157</shortName><identifier>ivo://CDS.VizieR/J/A+A/616/A157</identifier><altIdentifier>doi:10.26093/cds/vizier.36160157</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Leslie S.K.</name></creator><creator><name>Schinnerer E.</name></creator><creator><name>Groves B.</name></creator><creator><name>Sargent M.T.</name></creator><creator><name>Zamorani G.</name></creator><creator><name>Lang P.,Vardoulaki E.</name></creator><date role="Updated">2018-09-10T07:58:19Z</date><date role="Created">2018-09-07T07:55:59Z</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>photometry</subject><description>We evaluate dust-corrected far-ultraviolet (FUV) star formation rates (SFRs) for samples of star-forming galaxies at z~0 and z~0.7 and find significant differences between values obtained through corrections based on UV colour, from a hybrid mid-infrared (MIR) plus FUV relation, and from a radiative transfer based attenuation correction method. The performances of the attenuation correction methods are assessed by their ability to remove the dependency of the corrected SFR on inclination, as well as returning, on average, the expected population mean SFR. We find that combining MIR (rest-frame ~13um) and FUV luminosities gives the most inclination-independent SFRs and reduces the intrinsic SFR scatter of the methods we tested. However, applying the radiative transfer based method gives corrections to the FUV SFR that are inclination independent and in agreement with the expected SFRs at both z~0 and z~0.7. SFR corrections based on the UV-slope perform worse than the other two methods we tested. For our local sample, the UV-slope method works on average, but does not remove inclination biases. At z~0.7, we find that the UV-slope correction we used locally flattens the inclination dependence compared to the raw FUV measurements, but was not sufficient to correct for the large attenuation observed at z~0.7.</description><source format="bibcode">2018A&amp;A...616A.157L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/616/A157</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/616/A157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/616/A157</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/616/A157</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/616/A157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/616/A157</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/616/A157</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"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/616/A157/localsfr</name><description>SFRs of local galaxy sample</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>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logM</name><description>Stellar mass (log10)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logM</name><description>Error on stellar mass</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>1-cosi</name><description>? 1-cos(inclination)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_1-cosi</name><description>? Error on 1-cos(inclination)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>r50</name><description>Half-light radius g-band</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>n</name><description>Sersic index g-band</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logSFRFUVobs</name><description>FUV star formation rate, log(SFRFUV)</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logSFRFUVobs</name><description>Error on log(SFRFUV)</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logSFRFUVb</name><description>log(SFRFUV) corrected with beta</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logSFRFUVb</name><description>Error on log(SFRFUVb)</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logSFRFUVIR</name><description>? log(SFRFUV) corrected by UV+IR</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logSFRFUVIR</name><description>? Error on log(SFRFUVIR)</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logSFRFUVRT</name><description>? log(SFRFUV) corrected using RT</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logSFRFUVRT</name><description>? Error on log(SFRFUVRT)</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/616/A157/cosmosfr</name><description>SFRs of intermediate redshift galaxy sample</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>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logM</name><description>Stellar mass (log10)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logM</name><description>Error on stellar mass</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>1-cosi</name><description>1-cos(inclination)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_1-cosi</name><description>Error on 1-cos(inclination)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>r50</name><description>half-light radius I-band</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>n</name><description>Sersic index I-band</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logSFRUVobs</name><description>FUV star formation rate, log(SFRFUV)</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logSFRUVobs</name><description>Error on log(SFRFUV)</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logSFRUVb</name><description>? log(SFRFUV) corrected using beta</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_logSFRUVb</name><description>? 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