<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2018-02-08T08:14:30Z" 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>HD147379 b velocity curve</title><shortName>J/A+A/609/L5</shortName><identifier>ivo://CDS.VizieR/J/A+A/609/L5</identifier><altIdentifier>doi:10.26093/cds/vizier.36099005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Reiners A.</name></creator><creator><name>Ribas I.</name></creator><creator><name>Zechmeister M.</name></creator><creator><name>Caballero J.A.</name></creator><creator><name>Trifonov T.,Dreizler S.</name></creator><creator><name>Morales J.C.</name></creator><creator><name>Tal-Or L.</name></creator><creator><name>Lafarga M.</name></creator><creator><name>Quirrenbach A.,Amado P.J.</name></creator><creator><name>Kaminski A.</name></creator><creator><name>Jeffers S.V.</name></creator><creator><name>Aceituno J.</name></creator><creator><name>Bejar V.J.S.,Guardia J.</name></creator><creator><name>Guenther E.W.</name></creator><creator><name>Hagen H.-J.</name></creator><creator><name>Montes D.</name></creator><creator><name>Passegger V.M.,Seifert W.</name></creator><creator><name>Schweitzer A.</name></creator><creator><name>Cortes-Contreras M.</name></creator><creator><name>Abril M.,Alonso-Floriano F.J.</name></creator><creator><name>Ammler-von Eiff M.</name></creator><creator><name>Antona R.</name></creator><creator><name>Anglada-Escude G.,Anwand-Heerwart H.</name></creator><creator><name>Arroyo-Torres B.</name></creator><creator><name>Azzaro M.</name></creator><creator><name>Baroch D.</name></creator><creator><name>Barrado D.,Bauer F.F.</name></creator><creator><name>Becerril S.</name></creator><creator><name>Benitez D.</name></creator><creator><name>Berdinas Z.M.</name></creator><creator><name>Bergond G.,Bluemcke M.</name></creator><creator><name>Brinkmoeller M.</name></creator><creator><name>del Burgo C.</name></creator><creator><name>Cano J.</name></creator><creator><name>Cardenas Vazquez M.C.,Casal E.</name></creator><creator><name>Cifuentes C.</name></creator><creator><name>Claret A.</name></creator><creator><name>Colome J.</name></creator><creator><name>Czesla S.</name></creator><creator><name>Diez-Alonso E.,Feiz C.</name></creator><creator><name>Fernandez M.</name></creator><creator><name>Ferro I.M.</name></creator><creator><name>Fuhrmeister B.</name></creator><creator><name>Galadi-Enriquez D.,Garcia-Piquer A.</name></creator><creator><name>Garcia Vargas M.L.</name></creator><creator><name>Gesa L.</name></creator><creator><name>Gomez Galera V.,Gonzalez Hernandez J.I.</name></creator><creator><name>Gonzalez-Peinado R.</name></creator><creator><name>Groezinger U.</name></creator><creator><name>Grohnert S.,Guijarro A.</name></creator><creator><name>de Guindos E.</name></creator><creator><name>Gutierrez-Soto J.</name></creator><creator><name>Hatzes A.P.,Hauschildt P.H.</name></creator><creator><name>Hedrosa R.P.</name></creator><creator><name>Helmling J.</name></creator><creator><name>Henning Th.</name></creator><creator><name>Hermelo I.,Hernandez Arabi R.</name></creator><creator><name>Hernandez Castano L.</name></creator><creator><name>Hernandez Hernando F.,Herrero E.</name></creator><creator><name>Huber A.</name></creator><creator><name>Huke P.</name></creator><creator><name>Johnson E.N.</name></creator><creator><name>de Juan E.</name></creator><creator><name>Kim M.,Klein R.</name></creator><creator><name>Klueter J.</name></creator><creator><name>Klutsch A.</name></creator><creator><name>Kuerster M.</name></creator><creator><name>Labarga F.</name></creator><creator><name>Lamert A.,Lampon M.</name></creator><creator><name>Lara L.M.</name></creator><creator><name>Laun W.</name></creator><creator><name>Lemke U.</name></creator><creator><name>Lenzen R.</name></creator><creator><name>Launhardt R.,Lopez del Fresno M.</name></creator><creator><name>Lopez-Gonzalez M.J.</name></creator><creator><name>Lopez-Puertas M.,Lopez Salas J.F.</name></creator><creator><name>Lopez-Santiago J.</name></creator><creator><name>Luque R.</name></creator><creator><name>Magan Madinabeitia H.,Mall U.</name></creator><creator><name>Mancini L.</name></creator><creator><name>Mandel H.</name></creator><creator><name>Marfil E.</name></creator><creator><name>Marin Molina J.A.,Maroto Fernandez D.</name></creator><creator><name>Martin E.L.</name></creator><creator><name>Martin-Ruiz S.</name></creator><creator><name>Marvin C.J.</name></creator><creator><name>Mathar R.J.,Mirabet E.</name></creator><creator><name>Moreno-Raya M.E.</name></creator><creator><name>Moya A.</name></creator><creator><name>Mundt R.</name></creator><creator><name>Nagel E.</name></creator><creator><name>Naranjo V.,Nortmann L.</name></creator><creator><name>Nowak G.</name></creator><creator><name>Ofir A.</name></creator><creator><name>Oreiro R.</name></creator><creator><name>Palle E.</name></creator><creator><name>Panduro J.,Pascual J.</name></creator><creator><name>Pavlov A.</name></creator><creator><name>Pedraz S.</name></creator><creator><name>Perez-Calpena A.</name></creator><creator><name>Perez Medialdea D.,Perger M.</name></creator><creator><name>Perryman M.A.C.</name></creator><creator><name>Pluto M.</name></creator><creator><name>Rabaza O.</name></creator><creator><name>Ramon A.</name></creator><creator><name>Rebolo R.,Redondo P.</name></creator><creator><name>Reffert S.</name></creator><creator><name>Reinhart S.</name></creator><creator><name>Rhode P.</name></creator><creator><name>Rix H.-W.</name></creator><creator><name>Rodler F.,Rodriguez E.</name></creator><creator><name>Rodriguez-Lopez C.</name></creator><creator><name>Rodriguez Trinidad A.</name></creator><creator><name>Rohloff R.-R.,Rosich A.</name></creator><creator><name>Sadegi S.</name></creator><creator><name>Sanchez-Blanco E.</name></creator><creator><name>Sanchez Carrasco M.A.,Sanchez-Lopez A.</name></creator><creator><name>Sanz-Forcada J.</name></creator><creator><name>Sarkis P.</name></creator><creator><name>Sarmiento L.F.</name></creator><creator><name>Schaefer S.,Schmitt J.H.M.M.</name></creator><creator><name>Schiller J.</name></creator><creator><name>Schoefer P.</name></creator><creator><name>Solano E.</name></creator><creator><name>Stahl O.,Strachan J.B.P.</name></creator><creator><name>Stuermer J.</name></creator><creator><name>Suarez J.C.</name></creator><creator><name>Tabernero H.M.</name></creator><creator><name>Tala M.,Tulloch S.M.</name></creator><creator><name>Ulbrich R.-G.</name></creator><creator><name>Veredas G.</name></creator><creator><name>Vico Linares J.I.</name></creator><creator><name>Vilardell F.,Wagner K.</name></creator><creator><name>Winkler J.</name></creator><creator><name>Wolthoff V.</name></creator><creator><name>Xu W.</name></creator><creator><name>Yan F.</name></creator><creator><name>Zapatero Osorio M.R.</name></creator><date role="Updated">2018-03-12T09:03:21Z</date><date role="Created">2018-02-08T08:14:30Z</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>solar-system-planets</subject><subject>radial-velocity</subject><description>We report on the first star discovered to host a planet detected by radial velocity (RV) observations obtained within the CARMENES survey for exoplanets around M dwarfs. HD 147379 (V=8.9mag, M=0.58+/-0.08M_{sun}_), a bright M0.0 V star at a distance of 10.7pc, is found to undergo periodic RV variations with a semi-amplitude of K=5.1+/-0.4m/s and a period of P=86.54+/-0.06d. The RV signal is found in our CARMENES data, which were taken between 2016 and 2017, and is supported by HIRES/Keck observations that were obtained since 2000. The RV variations are interpreted as resulting from a planet of minimum mass m_P_sini=25+/-2M_{Earth}_, 1.5 times the mass of Neptune, with an orbital semi-major axis a=0.32au and low eccentricity (e&lt;0.13). HD 147379 b is orbiting inside the temperate zone around the star, where water could exist in liquid form. The RV time-series and various spectroscopic indicators show additional hints of variations at an approximate period of 21.1d (and its first harmonic), which we attribute to the rotation period of the star.</description><source format="bibcode">2018A&amp;A...609L...5R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/609/L5</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/577/A128">J/A+A/577/A128 : CARMENES input catalogue of M dwarfs. I</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/597/A47">J/A+A/597/A47 : CARMENES input catalogue of M dwarfs. II</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/609/L5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/609/L5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/609/L5</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/609/L5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/609/L5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/609/L5</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"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/609/L5/table1</name><description>HD147379 radial velocities</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>JD</name><description>Julian date of observation</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>Radial velocity uncertainty</description><unit>m/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>