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<ri:Resource created="2012-08-06T21:11:54Z" 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>PHASES diff. astrometry data archive. V.</title><shortName>J/AJ/140/1657</shortName><identifier>ivo://CDS.VizieR/J/AJ/140/1657</identifier><altIdentifier>doi:10.26093/cds/vizier.51401657</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Muterspaugh M.W.</name></creator><creator><name>Lane B.F.</name></creator><creator><name>Kulkarni S.R.</name></creator><creator><name>Konacki M.</name></creator><creator><name>Burke B.F.,Colavita M.M.</name></creator><creator><name>Shao M.</name></creator><creator><name>Hartkopf W.I.</name></creator><creator><name>Boss A.P.</name></creator><creator><name>Williamson M.</name></creator><date role="Updated">2017-10-13T15:42:05Z</date><date role="Created">2012-08-06T21:11:54Z</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>astrometry</subject><subject>interferometry</subject><description>The Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian planets orbited either the primary or secondary stars, perturbing their otherwise smooth Keplerian motions. Six binaries are presented that show evidence of substellar companions orbiting either the primary or secondary star. Of these six systems, the likelihoods of two of the detected perturbations to represent real objects are considered to be "high confidence," while the remaining four systems are less certain and will require continued observations for confirmation.</description><source format="bibcode">2010AJ....140.1657M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/140/1657</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/J/AJ/140/1579">J/AJ/140/1579 : PHASES diff. astrometry data archive. I. (Muterspaugh+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/1623">J/AJ/140/1623 : PHASES diff. astrometry data archive. II. 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