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<ri:Resource created="2015-06-18T07:50:54Z" 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>Period changes in SuperWASP eclipsing binaries</title><shortName>J/A+A/578/A136</shortName><identifier>ivo://CDS.VizieR/J/A+A/578/A136</identifier><altIdentifier>doi:10.26093/cds/vizier.35780136</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lohr M.E.</name></creator><creator><name>Norton A.J.</name></creator><creator><name>Payne S.G.</name></creator><creator><name>West R.G.</name></creator><creator><name>Wheatley P.J.</name></creator><date role="Updated">2017-10-13T15:41:59Z</date><date role="Created">2015-06-18T07:50:54Z</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>eclipsing-binary-stars</subject><subject>variable-stars</subject><subject>ccd-photometry</subject><description>Orbital period changes of binary stars may be caused by the presence of a third massive body in the system. Here we have searched the archive of the Wide Angle Search for Planets (SuperWASP) project for evidence of period variations in 13927 eclipsing binary candidates. Sinusoidal period changes, strongly suggestive of third bodies, were detected in 2% of cases; however, linear period changes were observed in a further 22% of systems. We argue on distributional grounds that the majority of these apparently linear changes are likely to reflect longer-term sinusoidal period variations caused by third bodies, and thus estimate a higher-order multiplicity fraction of 24% for SuperWASP binaries, in good agreement with other recent figures for the fraction of triple systems amongst binary stars in general.</description><source format="bibcode">2015A&amp;A...578A.136L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/578/A136</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></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface 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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>1SWASP</name><description>SuperWASP identifier (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>f_1SWASP</name><description>[d] Object is duplicate of neighbour(s)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000) from 1SWASP ID</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000) from 1SWASP ID</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Per</name><description>[10084/502168] Orbital period</description><unit>s</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Per</name><description>[0.0006/0.5] Uncertainty in orbital period</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pch</name><description>[-6.5/4.6] Period change from quadratic fit</description><unit>s/yr</unit><ucd>arith.rate;time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Pch</name><description>[9e-05/1] Uncertainty in period change</description><unit>s/yr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Qchi</name><description>Reduced {chi}^2^ for best quadratic O-C fit</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Type</name><description>Simbad column added by the CDS</description><ucd>meta.code;src.var</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/A+A/578/A136/sinus</name><description>SuperSWAP elcipsing binaries with sinusoidal period changes</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>1SWASP</name><description>SuperWASP identifier (JHHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>f_1SWASP</name><description>[d] Object is duplicate of neighbour(s)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000) from 1SWASP ID</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000) from 1SWASP ID</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Per</name><description>[10084/502168] Orbital period</description><unit>s</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Per</name><description>[9e-05/1] Uncertainty in orbital period</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lchi</name><description>Reduced {chi}^2^ for best linear O-C fit</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Qchi</name><description>Reduced {chi}^2^ for best quadratic O-C fit</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>