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<ri:Resource created="2003-05-30T22:30:16Z" 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>UV to radio SED of galaxies in Virgo cluster</title><shortName>J/A+A/402/37</shortName><identifier>ivo://CDS.VizieR/J/A+A/402/37</identifier><altIdentifier>doi:10.26093/cds/vizier.34020037</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boselli A.</name></creator><creator><name>Gavazzi G.</name></creator><creator><name>Sanvito G.</name></creator><date role="Updated">2017-06-26T11:49:09Z</date><date role="Created">2003-05-30T22:30:16Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>visible-astronomy</subject><subject>radio-sources</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>infrared-astronomy</subject><description>We present a multifrequency dataset for an optically-selected, volume-limited, complete sample of 118 late-type galaxies (&gt;=S0a) in the Virgo cluster. The database includes UV, visible, near-IR, mid-IR, far-IR, radio continuum photometric data as well as spectroscopic data of H{alpha}, CO and HI lines, homogeneously reduced, obtained from our own observations or compiled from the literature. Assuming the energy balance between the absorbed stellar light and that radiated in the IR by dust, we calibrate an empirical attenuation law suitable for correcting photometric and spectroscopic data of normal galaxies. The data, corrected for internal extinction, are used to construct the spectral energy distribution (SED) of each individual galaxy, and combined to trace the median SED of galaxies in various classes of morphological type and luminosity.</description><source format="bibcode">2003A&amp;A...402...37B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/402/37</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/121/507">J/A+AS/121/507 : Near-IR surface photometry of Virgo galaxies (Boselli+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/396/449">J/A+A/396/449 : H{alpha} surface photometry in Virgo (Gavazzi+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/41/421">J/A+AS/41/421 : 1.4GHz survey in the Virgo region (Kotanyi 1980)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/127/367">J/A+AS/127/367 : Virgo Photometry Catalogue (VPC) (Young+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/109/1608">J/AJ/109/1608 : Near-IR Surface Photometry in Virgo Spirals (Rauscher 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/111/143">J/ApJS/111/143 : Virgo cluster ultraviolet sources (Brosch+ 1997)</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/402/37</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/402/37</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/402/37</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/402/37</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/402/37</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/402/37</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>UV</waveband><waveband>Optical</waveband><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/402/37/table10</name><description>Bruzual-Charlot fitting models in the visible, corrected for dust extinction, for different templates (fluxes are given in Log(f(nu)/f(K))</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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