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<ri:Resource created="2014-04-08T13:13:03Z" 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>Light curves of HS Aqr, EG Cep, VW LMi, DU Boo</title><shortName>J/AJ/145/80</shortName><identifier>ivo://CDS.VizieR/J/AJ/145/80</identifier><altIdentifier>doi:10.26093/cds/vizier.51450080</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Djurasevic G.</name></creator><creator><name>Basturk O.</name></creator><creator><name>Latkovic O.</name></creator><creator><name>Yilmaz M.</name></creator><creator><name>Caliskan S.,Tanriverdi T.</name></creator><creator><name>Senavci H.V.</name></creator><creator><name>Kilicoglu T.</name></creator><creator><name>Ekmekci F.</name></creator><date role="Updated">2017-09-29T09:04:06Z</date><date role="Created">2014-04-08T13:13:03Z</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>We analyze new multicolor light curves for four close late-type binaries: HS Aqr, EG Cep, VW LMi, and DU Boo, in order to determine the orbital and physical parameters of the systems and estimate the distances. The analysis is done using the modeling code of G. Djurasevic, and is based on up-to-date measurements of spectroscopic elements. All four systems have complex, asymmetric light curves that we model by including bright or dark spots on one or both components. 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