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<ri:Resource created="2014-04-14T09:40:09Z" status="active" updated="2026-01-13T20:00:51Z" 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>STEREO magnetic chemically peculiar stars</title><shortName>J/MNRAS/420/757</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/420/757</identifier><altIdentifier>doi:10.26093/cds/vizier.74200757</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wraight K.T.</name></creator><creator><name>Fossati L.</name></creator><creator><name>Netopil M.</name></creator><creator><name>Paunzen E.</name></creator><creator><name>Rode-Paunzen M.,Bewsher D.</name></creator><creator><name>Norton A.J.</name></creator><creator><name>White G.J.</name></creator><date role="Updated">2026-01-13T20:00:51Z</date><date role="Created">2014-04-14T09:40:09Z</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>peculiar-variable-stars</subject><description>About 10% of upper main-sequence stars are characterized by the presence of chemical peculiarities, often found together with a structured magnetic field. The atmospheres of most of those chemically peculiar stars present surface spots, leading to photometric variability caused by rotational modulation. The study of the light curves of those stars therefore permits a precise measurement of their rotational period, which is important to study stellar evolution and to plan further detailed observations. We analysed the light curves of 1028 chemically peculiar stars obtained with the STEREO spacecraft. We present here the results obtained for the 337 magnetic chemically peculiar stars in our sample.</description><source format="bibcode">2012MNRAS.420..757W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/420/757</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/III/260">III/260 : General Catalogue of Ap and Am stars (Renson+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/429/119">J/MNRAS/429/119 : STEREO non-magnetic chemically peculiar stars (Paunzen+ 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>R09</name><description>Identification number by Renson &amp; Manfroid (2009A&amp;A...498..961R, Cat. 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