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<ri:Resource created="2013-02-07T09:16:07Z" status="active" updated="2025-06-13T15:25:00Z" 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>Distances and kinematics with CoRoT stars</title><shortName>J/A+A/550/A125</shortName><identifier>ivo://CDS.VizieR/J/A+A/550/A125</identifier><altIdentifier>doi:10.26093/cds/vizier.35500125</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gazzano J.-C.</name></creator><creator><name>Kordopatis G.</name></creator><creator><name>Deleuil M.</name></creator><creator><name>de Laverny P.</name></creator><creator><name>Recio-Blanco A.,Hill V.</name></creator><date role="Updated">2017-06-22T14:28:28Z</date><date role="Created">2013-02-07T09:16:07Z</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>infrared-photometry</subject><subject>stellar-distance</subject><description>We use kinematical and chemical properties of 754 CoRoT stars to characterise the stellar populations of the Milky Way disc in three beams close the Galactic plane. From the atmospheric parameters derived in Gazzano et al. (2010, Cat. J/A+A/523/A91) with the MATISSE algorithm, we derived stellar distances using isochrones. Combining these data with proper motions, we provide the complete kinematical description of stars in three CoRoT fields. 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