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<ri:Resource created="2014-06-05T09:12:53Z" 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>EPOCH Project. EROS-2 LMC periodic variables</title><shortName>J/A+A/566/A43</shortName><identifier>ivo://CDS.VizieR/J/A+A/566/A43</identifier><altIdentifier>doi:10.26093/cds/vizier.35660043</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kim D.-W.</name></creator><creator><name>Protopapas P.</name></creator><creator><name>Bailer-Jones C.A.L.</name></creator><creator><name>Byun Y.-I.</name></creator><creator><name>Chang S.-W.,Marquette J.-B.</name></creator><creator><name>Shin M.-S.</name></creator><date role="Updated">2017-12-22T05:33:21Z</date><date role="Created">2014-06-05T09:12:53Z</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>magellanic-clouds</subject><subject>surveys</subject><subject>variable-stars</subject><subject>ccd-photometry</subject><subject>infrared-astronomy</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>The EPOCH (EROS-2 periodic variable star classification using machine learning) project aims to detect periodic variable stars in the EROS-2 light curve database. In order to classify these variables, we first build a training set by compiling known variables in the Large Magellanic Could area from the OGLE and MACHO surveys. We crossmatch these variables with the EROS-2 sources and extract 22 variability features from 28,392 light curves of the corresponding EROS-2 sources. We then use Random Forests to classify the EROS-2 sources in the training set. We design the model to separate not only Delta Scuti stars, RR Lyraes, Cepheids, eclipsing binaries and long-period variables, the "superclasses", but also their subclasses, such as RRab, RRc, RRd and RRe for RR Lyraes, and similarly for the other variable types. We apply the trained model to the entire EROS-2 LMC database containing about 29 million sources and find 117,234 periodic variable candidates. Out of these 117,234 periodic variables, 55,285 have not been discovered by either OGLE or MACHO variability studies. This set comprises 1906 Delta Scuti stars, 6,607 RR Lyraes, 638 Cepheids, 178 Type II Cepheids, 34,562 eclipsing binaries and 11,394 long-period variables.</description><source format="bibcode">2014A&amp;A...566A..43K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/566/A43</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/II/247">II/247 : Variable Stars in the Large Magellanic Clouds (MACHO, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/49/223">J/AcA/49/223 : BVI photometry of OGLE LMC Cepheids (Udalski+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/50/307">J/AcA/50/307 : OGLE LMC BVI photometry (Udalski+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/53/93">J/AcA/53/93 : OGLE RR Lyrae in LMC (Soszynski+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/58/163">J/AcA/58/163 : VI light curves of LMC classical Cepheids (Soszynski+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/58/293">J/AcA/58/293 : Type-II and anomalous Cepheids in LMC (Soszynski+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/59/1">J/AcA/59/1 : VI light curves of LMC RR Lyrae stars (Soszynski+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/59/239">J/AcA/59/239 : VI light curves of LMC long-period variables (Soszynski+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/59/335">J/AcA/59/335 : VI light curves of LMC R CBr stars (Soszynski+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/60/1">J/AcA/60/1 : VI light curves of LMC delta Scuti stars (Poleski+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/60/179">J/AcA/60/179 : VI light curves of LMC double periodic variables (Poleski+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/61/103">J/AcA/61/103 : VI light curves of LMC eclipsing binaries (Szymanski+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/303/137">J/A+A/303/137 : EROS Variables: Cepheids in the bar of LMC (Beaulieu+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/377/945">J/A+A/377/945 : Variability and spectra of LMC giants (Cioni+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/495/249">J/A+A/495/249 : EROS-2 beat Cepheids in Magellanic Clouds (Marquette+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/536/A60">J/A+A/536/A60 : EROS-2 Long 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