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<ri:Resource created="2010-07-10T20:11:43Z" 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>UBVRI photometry in Be 15, Be 80 and NGC 2192</title><shortName>J/MNRAS/401/621</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/401/621</identifier><altIdentifier>doi:10.26093/cds/vizier.74010621</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tapia M.T.</name></creator><creator><name>Schuster W.J.</name></creator><creator><name>Michel R.</name></creator><creator><name>Chavarria-K. C.</name></creator><creator><name>Dias W.S.,Vazquez R.</name></creator><creator><name>Moitinho A.</name></creator><date role="Updated">2024-07-10T20:17:05Z</date><date role="Created">2010-07-10T20:11:43Z</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>open-star-clusters</subject><subject>ccd-photometry</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>kron-cousins-photometry</subject><description>The three open clusters Be 15, Be 80 and NGC 2192 have been observed using CCD UBV(RI)C photometry at the San Pedro Martir Observatory, Mexico within the framework of our open-cluster survey. The fundamental parameters of interstellar reddening, distance and age have been derived, and also the metallicity for NGC 2192 (solar metallicity has been assumed for the other two).</description><source format="bibcode">2010MNRAS.401..621T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/401/621</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/other/BASI/32.295">J/other/BASI/32.295 : CCD UBVRI phot. of Be 15, Cz 18, NGC 2401 (Sujatha+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/364/179">J/MNRAS/364/179 : BVI photometry of 8 open clusters (Carraro+, 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/MNRAS/401/621</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/401/621</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/401/621</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/401/621</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/401/621</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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