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<ri:Resource created="2008-09-12T12:18:05Z" 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>H{alpha} observations of UV-selected galaxies</title><shortName>J/ApJ/647/128</shortName><identifier>ivo://CDS.VizieR/J/ApJ/647/128</identifier><altIdentifier>doi:10.26093/cds/vizier.16470128</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Erb D.K.</name></creator><date role="Updated">2017-10-12T12:59:40Z</date><date role="Created">2008-09-12T12:18:05Z</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>ultraviolet-photometry</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><description>Using Halpha spectra of 114 rest-frame UV-selected galaxies at z~2, we compare inferred star formation rates (SFRs) with those determined from the UV continuum luminosity. After correcting for extinction using standard techniques based on the UV continuum slope, we find excellent agreement between the indicators, with &lt;SFR_Ha_&gt;=31M_{sun}_/yr and &lt;SFR_UV_&gt;=29M_{sun}_/yr. The agreement between the indicators suggests that the UV luminosity is attenuated by a typical factor of ~4.5 (ranging from no attenuation to a factor of 100 for the most obscured object in the sample), in good agreement with estimates of obscuration from X-ray, radio, and mid-IR data.</description><source format="bibcode">2006ApJ...647..128E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/647/128</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/MNRAS/300/303">J/MNRAS/300/303 : UV-selected galaxy redshift survey (Treyer+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/122/109">J/ApJS/122/109 : Galaxy structural parameters (Takamiya+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/549/820">J/ApJ/549/820 : H{alpha} flux of ACCG 114 galaxies (Couch+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/379/798">J/A+A/379/798 : ELAIS H{alpha} emitting galaxies (Pascual+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/586/794">J/ApJ/586/794 : Multiwavelength luminosities of galaxies (Bell, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/2002">J/AJ/127/2002 : Star Formation Rate of NFGS galaxies (Kewley+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/425/417">J/A+A/425/417 : Star formation rates of blue compact galaxies (Kong+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/604/141">J/ApJ/604/141 : H{alpha} fluxes in Cl J0023+0423B galaxies (Finn+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/630/206">J/ApJ/630/206 : H{alpha} data for 3 EDisCS galaxy clusters (Finn+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/117/227">J/PASP/117/227 : Properties of 101 galaxies from the NFGS (Kewley+, 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/ApJ/647/128</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/647/128</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/647/128</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/647/128</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/647/128</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/647/128</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/ApJ/647/128/table (Star formation rates results in the observed galaxies)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/647/128/table?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/647/128/table?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/647/128/table?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>13.4702917</ra><dec>12.3975694</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/9272 10383 11252 11424 11596 18271 18780 19036 19682 19717</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/647/128?format=ascii</footprint><waveband>UV</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/647/128/table</name><description>Star formation rates results in the observed galaxies</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>Name</name><description>Object name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>n_Name</name><description>[l] AGN (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>z</name><description>Redshift from H{alpha} line</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E(B-V)</name><description>The E(B-V) extinction (2)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FHa</name><description>Observed H{alpha} emission line flux in units of 10^-17^erg/s/cm^2^</description><unit>1e-20W.m**-2</unit><ucd>phot.flux;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LHa</name><description>Observed H{alpha} luminosity in units of 10^42^erg/s</description><unit>1e+35W</unit><ucd>phys.luminosity;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SFR0</name><description>Uncorrected SFR from H{alpha} flux (3)</description><unit>solMass/yr</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SFR1</name><description>SFR from H{alpha} flux (4)</description><unit>solMass/yr</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>F1500</name><description>Observed 1500 Angstrom magnitude (5)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L1500</name><description>Log of the 1500 Angstrom rest frame luminosity in units of erg/s/cm^2^/Hz</description><unit>log(mW.m**-2.Hz**-1)</unit><ucd>phys.luminosity;em.UV</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>USFR0</name><description>Uncorrected SFR from UV magnitude</description><unit>solMass/yr</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>USFR1</name><description>SFR from extinction-corrected UV magnitude</description><unit>solMass/yr</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SFR</name><description>? 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