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<ri:Resource created="2009-12-29T14:58:00Z" 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>Frequency analysis of HD 180642 (V1449 Aql)</title><shortName>J/A+A/506/111</shortName><identifier>ivo://CDS.VizieR/J/A+A/506/111</identifier><altIdentifier>doi:10.26093/cds/vizier.35060111</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Degroote P.</name></creator><creator><name>Briquet M.</name></creator><creator><name>Catala C.</name></creator><creator><name>Uytterhoeven K.</name></creator><creator><name>Lefever K.</name></creator><creator><name>Morel T.,Aerts C.</name></creator><creator><name>Carrier F.</name></creator><creator><name>Auvergne M.</name></creator><creator><name>Baglin A.</name></creator><creator><name>Michel E.</name></creator><date role="Updated">2017-06-27T06:38:39Z</date><date role="Created">2009-12-29T14:58:00Z</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>early-type-stars</subject><description>We present the CoRoT light curve of the beta Cep star HD 180642, assembled during the first long run of the space mission, as well as archival single-band photometry. Our goal is to analyse the detailed behaviour present in the light curve and interpret it in terms of excited-mode frequencies. After describing the noise properties in detail, we use various time series analyses and fitting techniques to model the CoRoT light curve, for various physical assumptions. We apply statistical goodness-of-fit criteria that allow us to select the most appropriate physical model fit to the data. We conclude that the light-curve model based on nonlinear resonant frequency and phase locking provides the best representation of the data. Interpretation of the residuals is dependent on the chosen physical model used to prewhiten the data. Our observational results constitute a fruitful starting point for detailed seismic stellar modelling of this large-amplitude and evolved beta Cep star.</description><source format="bibcode">2009A&amp;A...506..111D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/506/111</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/B/corot">B/corot : CoRoT observation log (CoRoT, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/361/245">J/A+A/361/245 : 6 new Beta Cep stars (Aerts, 2000)</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/506/111</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/506/111</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/506/111</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/506/111</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/506/111</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/506/111</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>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/506/111/table1</name><description>Results of frequency analysis of the first 200 frequencies</description><column><name>e_P</name><description>Error on phase</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><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>Seq</name><description>Frequency ID number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>f1</name><description>Frequency value</description><unit>d**-1</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_f1</name><description>Error on frequency value</description><unit>d**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f2</name><description>Frequency value (identical to f1)</description><unit>uHz</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_f2</name><description>Error on frequency value (identical to e_f1)</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>A</name><description>Ratio amplitude/average flux</description><ucd>phot.mag;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_A</name><description>Error on amplitude</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>P</name><description>]-0.5,0.5] Phase (rad/2{pi})</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SNR</name><description>Signal-to-noise ratio over 6d-1 interval</description><ucd>stat.snr;time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VR</name><description>Variance reduction</description><unit>%</unit><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AIC</name><description>Value of Akaike's Information Criterion</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BIC</name><description>Value of Bayesian Information Criterion</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/506/111/table2</name><description>Frequency table with fixed combinations between parent and daughter modes</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>A</name><description>Ratio amplitude/average flux</description><ucd>phot.mag;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f1</name><description>Frequency value</description><unit>d**-1</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f2</name><description>Frequency value (same as f1)</description><unit>uHz</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>P</name><description>]-0.5,0.5] Phase (rad/2{pi})</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ar</name><description>? Relative amplitude (logarithmic)</description><ucd>phot.mag;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ar</name><description>? Error on amplitude ratio</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pr</name><description>]-0.5,0.5]? Relative phase (rad/2{pi})</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Pr</name><description>]-0.5,0.5]? Error on relative phase</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNR</name><description>Signal-to-noise ratio over 6d-1 interval</description><ucd>stat.snr;time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VR</name><description>Variance reduction</description><unit>%</unit><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AIC</name><description>Value of Akaike's Information Criterion</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BIC</name><description>Value of Bayesian Information Criterion</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/506/111/tables</name><description>Variable amplitude/phase model for a1, a2, a3, a4, phi1, phi2, phi3 and phi4 (tables 3-10 of the paper)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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