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<ri:Resource created="2018-06-05T12:12:41Z" status="active" updated="2025-09-25T20:16:21Z" 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>Gaia DR1 and OGLE variable stars</title><shortName>J/AcA/66/433</shortName><identifier>ivo://CDS.VizieR/J/AcA/66/433</identifier><altIdentifier>doi:10.26093/cds/vizier.120660433</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Udalski A.</name></creator><creator><name>Soszynski I.</name></creator><creator><name>Skowron D.M.</name></creator><creator><name>Skowron J.</name></creator><creator><name>Pietrukowicz P.,Mroz P.</name></creator><creator><name>Poleski R.</name></creator><creator><name>Szymanski M.K.</name></creator><creator><name>Kozlowski S.</name></creator><creator><name>Wyrzykowski L.,Ulaczyk K.</name></creator><creator><name>Pawlak M.</name></creator><date role="Updated">2025-09-25T20:16:21Z</date><date role="Created">2018-06-05T12:12:41Z</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>variable-stars</subject><subject>astronomical-object-identification</subject><description>We present a comparison of the Gaia DR1 samples of pulsating variable stars - Cepheids and RR Lyr type - with the OGLE Collection of Variable Stars aiming at the characterization of the Gaia mission performance in the stellar variability domain. Out of 575 Cepheids and 2322 RR Lyr candidates from the Gaia DR1 samples located in the OGLE footprint in the sky, 559 Cepheids and 2302 RR Lyr stars are genuine pulsators of these types. The number of misclassified stars is low indicating reliable performance of the Gaia data pipeline. The completeness of the Gaia DR1 samples of Cepheids and RR Lyr stars is at the level of 60-75% as compared to the OGLE Collection dataset. This level of completeness is moderate and may limit the applicability of the Gaia data in many projects.</description><source format="bibcode">2016AcA....66..433U</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AcA/66/433</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/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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