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<ri:Resource created="2009-07-29T06:12:29Z" 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>Physical properties of VVDS galaxies</title><shortName>J/A+A/495/53</shortName><identifier>ivo://CDS.VizieR/J/A+A/495/53</identifier><altIdentifier>doi:10.26093/cds/vizier.34950053</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lamareille F.</name></creator><creator><name>Brinchmann J.</name></creator><creator><name>Contini T.</name></creator><creator><name>Walcher C.J.</name></creator><creator><name>Charlot S.,Perez-Montero E.</name></creator><creator><name>Zamorani G.</name></creator><creator><name>Pozzetti L.</name></creator><creator><name>Bolzonella M.</name></creator><creator><name>Garilli B.,Paltani S.</name></creator><creator><name>Bongiorno A.</name></creator><creator><name>Le Fevre O.</name></creator><creator><name>Bottini D.</name></creator><creator><name>Le Brun V.</name></creator><creator><name>Maccagni D.,Scaramella R.</name></creator><creator><name>Scodeggio M.</name></creator><creator><name>Tresse L.</name></creator><creator><name>Vettolani G.</name></creator><creator><name>Zanichelli A.,Adami C.</name></creator><creator><name>Arnouts S.</name></creator><creator><name>Bardelli S.</name></creator><creator><name>Cappi A.</name></creator><creator><name>Ciliegi P.</name></creator><creator><name>Foucaud S.,Franzetti P.</name></creator><creator><name>Gavignaud I.</name></creator><creator><name>Guzzo L.</name></creator><creator><name>Ilbert O.</name></creator><creator><name>Iovino A.</name></creator><creator><name>McCracken H.J.,Marano B.</name></creator><creator><name>Marinoni C.</name></creator><creator><name>Mazure A.</name></creator><creator><name>Meneux B.</name></creator><creator><name>Merighi R.</name></creator><creator><name>Pello R.,Pollo A.</name></creator><creator><name>Radovich M.</name></creator><creator><name>Vergani D.</name></creator><creator><name>Zucca E.</name></creator><creator><name>Romano A.</name></creator><creator><name>Grado A.,Limatola L.</name></creator><date role="Updated">2009-07-29T06:18:59Z</date><date role="Created">2009-07-29T06:12:29Z</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>surveys</subject><subject>galaxies</subject><subject>spectroscopy</subject><subject>line-intensities</subject><description>We want to derive the mass-metallicity relation of star-forming galaxies up to z~0.9, using data from the VIMOS VLT Deep Survey. The mass-metallicity relation is commonly understood as the relation between the stellar mass and the gas-phase oxygen abundance. Automatic measurement of emission-line fluxes and equivalent widths have been performed on the full spectroscopic sample of the VIMOS VLT Deep Survey. This sample is divided into two sub-samples depending on the apparent magnitude selection: wide (I_AB_&lt;22.5) and deep (I_AB_&lt;24). These two samples span two different ranges of stellar masses. Emission-line galaxies have been separated into star-forming galaxies and active galactic nuclei using emission line ratios. For the star-forming galaxies the emission line ratios have also been used to estimate gas-phase oxygen abundance, using empirical calibrations renormalized in order to give consistent results at low and high redshifts. The stellar masses have been estimated by fitting the whole spectral energy distributions with a set of stellar population synthesis models.</description><source format="bibcode">2009A&amp;A...495...53L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/495/53</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/286">II/286 : VIRMOS deep imaging survey. VVDS-F02 cat. (VIRMOS team+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/250">III/250 : The VIMOS VLT deep survey (VVDS-DEEP) (Le Fevre+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/428/1043">J/A+A/428/1043 : Redshifts from VIMOS VLT Deep Survey (Le Fevre+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/413">J/A+A/439/413 : XMDS/VVDS 4{sigma} catalogue (Chiappetti+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/457/79">J/A+A/457/79 : VVDS-DEEP: faint type-1 AGN sample (Gavignaud+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/463/519">J/A+A/463/519 : VVDS-VLA Deep Field: 610 MHz catalog (Bondi+, 2007)</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/495/53</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/495/53</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/495/53</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/495/53</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/495/53</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/495/53</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/A+A/495/53/catalog (Emission-line measurements, spectral indices, and derived physical properties of galaxies observed in the VIMOS/VLT Deep Survey (VVDS))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/495/53/catalog?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/495/53/catalog?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/495/53/catalog?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>52.97644</ra><dec>-27.78226</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/4759 6522 6/17683 17686 17689 17692 19027 19030-19033 19035 27250-27251 27256-27257 35935 35957</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/495/53?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/495/53/catalog</name><description>Emission-line measurements, spectral indices, and derived physical properties of galaxies observed in the VIMOS/VLT Deep Survey (VVDS)</description><column><name>VVDS</name><description>VVDS identification number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>primary</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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