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<ri:Resource created="2014-03-04T11:44:12Z" 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>BV(RI)c light curves of V1043 Cas</title><shortName>J/AJ/145/14</shortName><identifier>ivo://CDS.VizieR/J/AJ/145/14</identifier><altIdentifier>doi:10.26093/cds/vizier.51450014</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Samec R.G.</name></creator><creator><name>Smith P.M.</name></creator><creator><name>Chamberlain H.</name></creator><creator><name>Faulkner D.R.</name></creator><creator><name>Van Hamme W.</name></creator><date role="Updated">2017-06-30T05:47:45Z</date><date role="Created">2014-03-04T11:44:12Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>Complete Bessel BVR_c_I_c_ light curves of V1043 Cassiopeia [2MASS J00371195+5301324, Mis V1292, USNO-A2.0 1425-00875743, {alpha}(2000)=00^h^37^m^11.95^s^, {delta}(2000)=+53{deg}01'32.5"] are analyzed. The system is a member of the small group of pre-contact W UMa binaries (PCWBs). Its light curve has the appearance of an Algol (EA) light curve, however it is made up of dwarf solar type components in a detached mode with a period of only 0.6616days. The analysis includes a period study, an improved ephemeris, a mass ratio search, and a simultaneous BVR_c_I_c_ Wilson-Devinney solution. We document about 20 other PCWBs given in the literature. Several have RS CVn-like properties.</description><source format="bibcode">2013AJ....145...14S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/145/14</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/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/124/693">J/PASP/124/693 : HO Psc UBV(RI)c light curves (Samec+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5969">J/other/IBVS/5969 : 80th name-list of variable stars. I. 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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>Dmag</name><description>Differential magnitude in Filter (1)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HJD</name><description>Heliocentric Julian Date (HJD-2455400)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flt</name><description>[BVRI] Filter (B, V, Rc, or Ic)</description><ucd>meta.id;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>