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<ri:Resource created="2024-06-13T08:03:12Z" 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>TESS catalog of 1322 contact binary candidates</title><shortName>J/AJ/167/192</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/192</identifier><altIdentifier>doi:10.26093/cds/vizier.51670192</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ding Xu</name></creator><creator><name>Song Z.</name></creator><creator><name>Wang C.</name></creator><creator><name>Ji K.</name></creator><date role="Updated">2024-11-07T20:09:08Z</date><date role="Created">2024-06-13T08:03:12Z</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>multiple-stars</subject><subject>novae</subject><subject>visible-astronomy</subject><subject>eclipsing-binary-stars</subject><subject>spectroscopic-binary-stars</subject><description>A contact binary may be the progenitor of a red nova that eventually produces a merger event and have a cut-off period of around 0.2days. Therefore, a large number of contact binaries is needed to search for the progenitor of red novae and to study the characteristics of short-period contact binaries. In this paper, we employ the Phoebe program to generate a large number of light curves based on the fundamental parameters of contact binaries. Using these light curves as samples, an autoencoder model is trained, which can reconstruct the light curves of contact binaries very well. When the error between the output light curve from the model and the input light curve is large, it may be due to other types of variable stars. The goodness of fit (R2) between the output light curve from the model and the input light curve is calculated. Based on the thresholds for global goodness of fit (R2), period, range magnitude, and local goodness of fit (R2), a total of 1322 target candidates were obtained.</description><source format="bibcode">2024AJ....167..192D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/192</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><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/83">J/AJ/141/83 : Kepler Mission. I. Eclipsing binaries in DR1 (Prsa+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/68">J/AJ/151/68 : Kepler Mission. VII. Eclipsing binaries in DR3 (Kirk+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/66/405">J/AcA/66/405 : Galactic bulge eclipsing &amp; ellipsoidal bin (Soszynski+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/465/4678">J/MNRAS/465/4678 : 9380 contact binaries from CRTS VSC (Marsh+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/237/28">J/ApJS/237/28 : WISE catalog of periodic variable stars (Chen+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/249/18">J/ApJS/249/18 : The ZTF catalog of periodic variable stars (Chen+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/254/10">J/ApJS/254/10 : Compilation of W UMa stars (Latkovic+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/164/202">J/AJ/164/202 : Extremely Low Mass Ratio Contact Bin I. 10 systems (Li+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/258/16">J/ApJS/258/16 : TESS Eclipsing Binary stars. 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