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<ri:Resource created="2020-08-04T13:45:49Z" status="active" updated="2026-03-17T20:08:36Z" 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>Calibration sample UBV and GALEX photometry</title><shortName>J/other/PASA/37.</shortName><identifier>ivo://CDS.VizieR/J/other/PASA/37.22</identifier><altIdentifier>doi:10.26093/cds/vizier/ds/dhkcc</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bilir S.</name></creator><creator><name>Alan N.</name></creator><creator><name>Guctekin Tuncel S.</name></creator><creator><name>Celebi M.</name></creator><creator><name>Yontan T.</name></creator><creator><name>Plevne O.,Ak S.</name></creator><creator><name>Ak T.</name></creator><creator><name>Karaali S.</name></creator><date role="Updated">2026-03-17T20:08:36Z</date><date role="Created">2020-08-04T13:45:49Z</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>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>ultraviolet-photometry</subject><subject>metallicity</subject><description>We derive transformation equations between GALEX and UBV colours by using the reliable data of 556 stars. We present two sets of equations: as a function of (only) luminosity class and as a function of both luminosity class and metallicity. The metallicities are provided from the literature, while the luminosity classes are determined by using the PARSEC mass tracks in this study. Small colour residuals and high squared correlation coefficients promise accurate derived colours. The application of the transformation equations to 70 stars with reliable data shows that the metallicity plays an important role in estimation of more accurate colours.</description><source format="bibcode">2020PASA...37...22B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/PASA/37.22</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/A+A/530/A15">J/A+A/530/A15 : Abundances of 94 stars (Nissen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/140">J/ApJ/743/140 : Abundances (Be,alpha) in metal-poor stars (Boesgaard+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/64">J/ApJ/753/64 : Detailed abundances for 97 metal-poor stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/552/A128">J/A+A/552/A128 : Stellar abundances of neutron-capture elements</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/434/1422">J/MNRAS/434/1422 : Atmospheric param. of 169 FGKM stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A71">J/A+A/562/A71 : Chemical abundances of solar neighbourhood dwarfs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/580/A24">J/A+A/580/A24 : Abundances in dwarfs, subgiants and giants (da Silva+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/582/A81">J/A+A/582/A81 : Gaia FGK benchmark stars: abundances (Jofre+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/588/A98">J/A+A/588/A98 : Metallicities and abundances of evolved stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/222/19">J/ApJS/222/19 : KPNO spectroscopy of G + K dwarfs HIP stars (Kim+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/225/32">J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/606/A94">J/A+A/606/A94 : Chemical abundances of 1059 FGK stars (Delgado Mena+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/21">J/AJ/153/21 : Abundances in the local region. 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F, G, and K dwarfs</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/other/PASA/37.22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/PASA/37.22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/PASA/37.22</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/other/PASA/37.22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/other/PASA/37.22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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