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<ri:Resource created="2011-02-18T15:51:57Z" 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>JHKLM light curves of WR 140</title><shortName>J/PAZh/37/34</shortName><identifier>ivo://CDS.VizieR/J/PAZh/37/34</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Taranova O.G.</name></creator><creator><name>Shenavrin V.I.</name></creator><date role="Updated">2017-06-01T08:52:46Z</date><date role="Created">2011-02-18T15:51:57Z</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>variable-stars</subject><subject>infrared-photometry</subject><description>We present the results of our infrared observations of WR 140 (=V1687 Cyg) in 2001-2010.</description><source format="bibcode">2011PAZh...37...34T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/37/34</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/AZh/79/1118">J/AZh/79/1118 : JHKLM photometry of FG Sge (Taranova+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/30/605">J/PAZh/30/605 : JHKLM photometry for carbon stars (Taranova+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/32/866">J/PAZh/32/866 : JHKLM photometry for 22 hot stars (Taranova+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/33/657">J/PAZh/33/657 : JHKLM photometry of eight planetary nebulae (Taranova+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/36/144">J/PAZh/36/144 : JHKLM photometry of 3 RV Tau supergiants (Taranova+, 2010)</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/PAZh/37/34</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PAZh/37/34</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PAZh/37/34</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PAZh/37/34</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/PAZh/37/34</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PAZh/37/34</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><spectral>3.533079825982027e-20 1.7798557115773645e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/PAZh/37/34/table1</name><description>Results of our infrared photometry for WR 140 (=V1687 Cyg), 2001-2010</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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