<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2015-03-09T13:46:32Z" 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/HIRES radial velocities for HD 97658</title><shortName>J/ApJ/772/L2</shortName><identifier>ivo://CDS.VizieR/J/ApJ/772/L2</identifier><altIdentifier>doi:10.26093/cds/vizier.17729002</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dragomir D.</name></creator><creator><name>Matthews J.M.</name></creator><creator><name>Eastman J.D.</name></creator><creator><name>Cameron C.</name></creator><creator><name>Howard A.W.,Guenther D.B.</name></creator><creator><name>Kuschnig R.</name></creator><creator><name>Moffat A.F.J.</name></creator><creator><name>Rowe J.F.</name></creator><creator><name>Rucinski S.M.,Sasselov D.</name></creator><creator><name>Weiss W.W.</name></creator><date role="Updated">2017-06-20T13:17:34Z</date><date role="Created">2015-03-09T13:46:32Z</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>radial-velocity</subject><subject>multiple-stars</subject><description>Through photometric monitoring of the extended transit window of HD 97658b with the MOST space telescope, we have found that this exoplanet transits with an ephemeris consistent with that predicted from radial velocity measurements. The mid-transit times are 5.6{sigma} earlier than those of the unverified transit-like signals reported in 2011, and we find no connection between the two sets of events. The transit depth together with our determined stellar radius (R_{star}_=0.703_-0.034_^+0.039^R_{sun}_) indicates a 2.34_-0.15_^0.18^R_{Earth}_ super-Earth. When combined with the radial velocity determined mass of 7.86+/-0.73M_{Earth}_, our radius measure allows us to derive a planet density of 3.44_-0.82_^+0.91^g/cm3. Models suggest that a planet with our measured density has a rocky core that is enveloped in an atmosphere composed of lighter elements. The star of the HD 97658 system is the second brightest known to host a transiting super-Earth, facilitating follow-up studies of this not easily daunted, warm and likely volatile-rich exoplanet.</description><source format="bibcode">2013ApJ...772L...2D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/772/L2</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/ApJ/759/L41">J/ApJ/759/L41 : New radial velocities of HD 97658 (Dragomir+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/37">J/ApJ/754/37 : HD 192263 radial velocities and photometry (Dragomir+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A114">J/A+A/533/A114 : Transit of super-Earth 55 Cnc e (Demory+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/123/412">J/PASP/123/412 : Exoplanet Orbit Database (Wright+, 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/ApJ/772/L2</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/772/L2</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/772/L2</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/772/L2</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/772/L2</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/772/L2</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/772/L2/table1</name><description>Radial velocities for HD 97658</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 (BJD-2440000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[-12.7/12.7] Radial velocity</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[0.4/1.7] Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>