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<ri:Resource created="2012-07-06T10:35:00Z" 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>Keck radial velocities of GJ 876</title><shortName>J/ApJ/719/890</shortName><identifier>ivo://CDS.VizieR/J/ApJ/719/890</identifier><altIdentifier>doi:10.26093/cds/vizier.17190890</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rivera E.J.</name></creator><creator><name>Laughlin G.</name></creator><creator><name>Butler R.P.</name></creator><creator><name>Vogt S.S.</name></creator><creator><name>Haghighipour N.,Meschiari S.</name></creator><date role="Updated">2017-06-29T08:55:44Z</date><date role="Created">2012-07-06T10:35:00Z</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>radial-velocity</subject><subject>solar-system-planets</subject><description>Continued radial velocity (RV) monitoring of the nearby M4V red dwarf star GJ 876 with Keck/High Resolution Echelle Spectrograph has revealed the presence of a Uranus-mass fourth planetary companion in the system. The new planet has a mean period of P_e_=126.6 days (over the 12.6-year baseline of the RV observations), and a minimum mass of m_e_sini_e_=12.9+/-1.7M_{earth}_. The detection of the new planet has been enabled by significant improvements to our RV data set for GJ 876. The data have been augmented by 36 new high-precision measurements taken over the past five years. In addition, the precision of all of the Doppler measurements have been significantly improved by the incorporation of a high signal-to-noise template spectrum for GJ 876 into the analysis pipeline. Implementation of the new template spectrum improves the internal rms errors for the velocity measurements taken during 1998-2005 from 4.1m/s to 2.5m/s.</description><source format="bibcode">2010ApJ...719..890R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/719/890</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/III/254">III/254 : 2nd Cat. of Radial Velocities with Astrometric Data (Kharchenko+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/213">III/213 : General Catalog of mean radial velocities (Barbier-Brossat+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/184">III/184 : 3rd Bibliog. Cat. of Stellar Radial Vel. (Barbier-Brossat+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/A21">J/A+A/511/A21 : Radial velocities of GJ876 planetary system (Correia+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/693/1084">J/ApJ/693/1084 : Ten new and updated multiplanet systems (Wright+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/646/505">J/ApJ/646/505 : Catalog of nearby exoplanets (Butler+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/634/625">J/ApJ/634/625 : Radial velocities and photometry of GJ 876 (Rivera+, 2005)</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/ApJ/719/890</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/719/890</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/719/890</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/719/890</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/719/890</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/719/890</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/ApJ/719/890/table1</name><description>Measured velocities for GJ 876 (Keck)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BJD</name><description>Barycentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RV</name><description>Radial velocity</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RV</name><description>Uncertainty in RV</description><unit>m/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>