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<ri:Resource created="2010-05-04T08:26:40Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>HARPS RV curves of HD125612, HD215497, HIP5158</title><shortName>J/A+A/512/A48</shortName><identifier>ivo://CDS.VizieR/J/A+A/512/A48</identifier><altIdentifier>doi:10.26093/cds/vizier.35120048</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lo Curto G.</name></creator><creator><name>Mayor M.</name></creator><creator><name>Benz W.</name></creator><creator><name>Bouchy F.</name></creator><creator><name>Lovis C.</name></creator><creator><name>Moutou C.</name></creator><creator><name>Naef D.,Pepe F.</name></creator><creator><name>Queloz D.</name></creator><creator><name>Santos N.C.</name></creator><creator><name>Segransan D.</name></creator><creator><name>Udry S.</name></creator><date role="Updated">2017-06-27T06:37:30Z</date><date role="Created">2010-05-04T08:26:40Z</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>solar-system-planets</subject><subject>radial-velocity</subject><description>We present the detections of three multiple systems within the HARPS volume-limited sample. Among the six planets discussed in this paper we have identified a "super-Earth" planet with a minimum mass of 6.6M_{Earth}_ and a "Neptune" planet with minimum mass of 18M_{Earth}_, both orbiting their parent stars within a distance of 0.05AU and a period of approximately four days. These detections strengthen the argument that low-mass planets are primarily found in multiple-planetary systems.</description><source format="bibcode">2010A&amp;A...512A..48L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/512/A48</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/474/293">J/A+A/474/293 : Radial velocities of GJ 674 (Bonfils+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/469/L43">J/A+A/469/L43 : Radial velocities of Gl 581 (Udry+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/496/513">J/A+A/496/513 : RV of 6 stars with long-period giant planets (Moutou+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/496/521">J/A+A/496/521 : Radial velocities of HD45364 (Correia+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/496/527">J/A+A/496/527 : Radial velocity of HD 47186 and HD 181433 (Bouchy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/507/487">J/A+A/507/487 : GJ 581 radial velocity curve (Mayor+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A46">J/A+A/512/A46 : Radial velocities of BD-08 2823 (Hebrard+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A47">J/A+A/512/A47 : Radial velocities of 3 stars with giant planets (Santos+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/523/A15">J/A+A/523/A15 : RV data for the 8 targets (Naef+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A111">J/A+A/526/A111 : HD 85390, 90156 and 103197 radial velocity (Mordasini+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A112">J/A+A/526/A112 : Radial velocities of HARPS metail-poor sample (Santos+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A141">J/A+A/526/A141 : HIP 85647 &amp; Gl 676A radial velocities (Forveille+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A63">J/A+A/527/A63 : 7 new HARPS planetary systems radial velocities (Moutou+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/528/A112">J/A+A/528/A112 : Radial velocities of HD 10180 (Lovis+, 2011)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/512/A48</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/512/A48</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/512/A48</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/512/A48</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/512/A48</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/512/A48</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/512/A48/hd125612</name><description>HD 125612 radial velocity measured</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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