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<ri:Resource created="2013-10-03T08:54:05Z" 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>RX J2117.1+3412 (V2027 Cyg) light curves</title><shortName>J/A+A/558/A63</shortName><identifier>ivo://CDS.VizieR/J/A+A/558/A63</identifier><altIdentifier>doi:10.26093/cds/vizier.35580063</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chang H.-K.</name></creator><creator><name>Shih I.-C.</name></creator><creator><name>Liu C.-Y.</name></creator><creator><name>Fan T.</name></creator><creator><name>Wu Y.-S.</name></creator><creator><name>Roques F.,Doressoundiram A.</name></creator><creator><name>Fernandez A.</name></creator><creator><name>Christophe B.</name></creator><creator><name>Dauny F.</name></creator><date role="Updated">2017-07-03T14:25:52Z</date><date role="Created">2013-10-03T08:54:05Z</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>white-dwarf-stars</subject><subject>photometry</subject><description>We report the effort to search for white dwarf p-mode oscillations in RX J2117.1+3412 (V2027 Cyg), a GW Vir star. The data were taken with Miosotys, a multi-fiber photometer, mounted on the 1.93-m telescope at Observatoire de Haute-Provence (OHP) with a 20-Hz cadence in May 2010 and June 2012. Two intriguing signatures at 1.2081Hz and 2.5852Hz were found at 3.8{sigma} and 3.5{sigma} significance levels, respectively. However, possible atmospheric effects cannot be ruled out. If these two features are not real, the 3{sigma} upper limit of the relative amplitude for the possible oscillations in the frequency range from 1 to 10Hz is estimated to be about 6x10^-4^. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MJD</name><description>Modified Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Int</name><description>Intensity, CCD recorded readings</description><unit>ct</unit><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/558/A63/0524r</name><description>Reference light curve on May 24, 2010</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MJD</name><description>Modified Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Int</name><description>Intensity, CCD recorded readings</description><unit>ct</unit><ucd>spect.line.intensity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/558/A63/0617t</name><description>V2027 Cyg light curve on June 17, 2012</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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