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<ri:Resource created="2019-07-05T09:27:52Z" 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>Radial velocities of K2-291 with HIRES &amp; HARPS-N</title><shortName>J/AJ/157/116</shortName><identifier>ivo://CDS.VizieR/J/AJ/157/116</identifier><altIdentifier>doi:10.26093/cds/vizier.51570116</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kosiarek M.R.</name></creator><creator><name>Blunt S.</name></creator><creator><name>Lopez-Morales M.</name></creator><creator><name>Crossfield I.J.M.</name></creator><creator><name>Sinukoff E.,Petigura E.A.</name></creator><creator><name>Gonzales E.J.</name></creator><creator><name>Poretti E.</name></creator><creator><name>Malavolta L.</name></creator><creator><name>Howard A.W.,Isaacson H.</name></creator><creator><name>Haywood R.D.</name></creator><creator><name>Ciardi D.R.</name></creator><creator><name>Bristow M.</name></creator><creator><name>Cameron A.C.,Charbonneau D.</name></creator><creator><name>Dressing C.D.</name></creator><creator><name>Figueira P.</name></creator><creator><name>Fulton B.J.</name></creator><creator><name>Hardee B.J.,Hirsch L.A.</name></creator><creator><name>Latham D.W.</name></creator><creator><name>Mortier A.</name></creator><creator><name>Nava C.</name></creator><creator><name>Schlieder J.E.,Vanderburg A.</name></creator><creator><name>Weiss L.</name></creator><creator><name>Bonomo A.S.</name></creator><creator><name>Bouchy F.</name></creator><creator><name>Buchhave L.A.</name></creator><creator><name>Coffinet A.,Damasso M.</name></creator><creator><name>Dumusque X.</name></creator><creator><name>Lovis C.</name></creator><creator><name>Mayor M.</name></creator><creator><name>Micela G.</name></creator><creator><name>Molinari E.,Pepe F.</name></creator><creator><name>Phillips D.</name></creator><creator><name>Piotto G.</name></creator><creator><name>Rice K.</name></creator><creator><name>Sasselov D.</name></creator><creator><name>Segransan D.,Sozzetti A.</name></creator><creator><name>Udry S.</name></creator><creator><name>Watson C.</name></creator><date role="Updated">2019-07-24T11:33:55Z</date><date role="Created">2019-07-05T09:27:52Z</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>exoplanets</subject><subject>multiple-stars</subject><description>K2-291 is a solar-type star with a radius of R_*_=0.899+/-0.034 R_{sun}_ and mass of M_*_=0.934+/-0.038 M_{sun}_. From the K2 C13 data, we found one super-Earth planet (R_p_=1.589_-0.072_^+0.095^ R_{Earth}_) transiting this star on a short period orbit (P=2.225177_-6.8e-5_^+6.6e-5^ days). We followed this system up with adaptive-optic imaging and spectroscopy to derive stellar parameters, search for stellar companions, and determine a planet mass. From our 75 radial velocity measurements using High Resolution Echelle Spectrometer on Keck I and High Accuracy Radial velocity Planet Searcher in the northern hemisphere on Telescopio Nazionale Galileo, we constrained the mass of K2-291 b to M_p_=6.49+/-1.16 M_{Earth}_. We found it necessary to model correlated stellar activity radial velocity signals with a Gaussian process (GP) in order to more accurately model the effect of stellar noise on our data; the addition of the GP also improved the precision of this mass measurement. With a bulk density of {rho}=8.84_-2.03_^+2.50^ g/cm^3^, the planet is consistent with an Earth-like rock/iron composition and no substantial gaseous envelope. Such an envelope, if it existed in the past, was likely eroded away by photoevaporation during the first billion years of the star's lifetime.</description><source format="bibcode">2019AJ....157..116K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/157/116</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/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/20">J/ApJS/210/20 : Small Kepler planets radial velocities (Marcy+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/52">J/AJ/157/52 : Radial velocity observations in super-Earth systems</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/AJ/157/116</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/157/116</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/157/116</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/157/116</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/157/116</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/157/116</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/AJ/157/116/table2</name><description>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>HJD</name><description>Heliocentric Julian Date at UTC</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RV</name><description>[-16.88/25150.7] Radial velocity</description><unit>m/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_RV</name><description>[0.98/4.73] Uncertainty in RV</description><unit>m/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SHK</name><description>[0.2131/0.2859] Ca II H&amp;K line emission indicator</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Inst</name><description>Instrument (1)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column></table></schema></tableset></ri:Resource>