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<ri:Resource created="2021-03-23T08:20:10Z" 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 velocity &amp; photometry of HD106315 &amp; GJ9827</title><shortName>J/AJ/161/47</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/47</identifier><altIdentifier>doi:10.26093/cds/vizier.51610047</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kosiarek M.R.</name></creator><creator><name>Berardo D.A.</name></creator><creator><name>Crossfield I.J.M.</name></creator><creator><name>Laguna C.</name></creator><creator><name>Piaulet C.,Akana Murphy J.M.</name></creator><creator><name>Howell S.B.</name></creator><creator><name>Henry G.W.</name></creator><creator><name>Isaacson H.</name></creator><creator><name>Fulton B.,Weiss L.M.</name></creator><creator><name>Petigura E.A.</name></creator><creator><name>Behmard A.</name></creator><creator><name>Hirsch L.A.</name></creator><creator><name>Teske J.</name></creator><creator><name>Burt J.A.,Mills S.M.</name></creator><creator><name>Chontos A.</name></creator><creator><name>Mocnik T.</name></creator><creator><name>Howard A.W.</name></creator><creator><name>Werner M.</name></creator><creator><name>Livingston J.H.,Krick J.</name></creator><creator><name>Beichman C.</name></creator><creator><name>Gorjian V.</name></creator><creator><name>Kreidberg L.</name></creator><creator><name>Morley C.,Christiansen J.L.</name></creator><creator><name>Morales F.Y.</name></creator><creator><name>Scott N.J.</name></creator><creator><name>Crane J.D.</name></creator><creator><name>Wang S.X.,Shectman S.A.</name></creator><creator><name>Rosenthal L.J.</name></creator><creator><name>Grunblatt S.K.</name></creator><creator><name>Rubenzahl R.A.</name></creator><creator><name>Dalba P.A.,Giacalone S.</name></creator><creator><name>Villanueva C.D.</name></creator><creator><name>Liu Q.</name></creator><creator><name>Dai F.</name></creator><creator><name>Hill M.L.</name></creator><creator><name>Rice M.,Kane S.R.</name></creator><creator><name>Mayo A.W.</name></creator><date role="Updated">2022-09-30T21:41:06Z</date><date role="Created">2021-03-23T08:20:10Z</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>exoplanets</subject><subject>radial-velocity</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>HD106315 and GJ9827 are two bright, nearby stars that host multiple super-Earths and sub-Neptunes discovered by K2 that are well suited for atmospheric characterization. We refined the planets ephemerides through Spitzer transits, enabling accurate transit prediction required for future atmospheric characterization through transmission spectroscopy. Through a multiyear high-cadence observing campaign with Keck/High Resolution Echelle Spectrometer and Magellan/Planet Finder Spectrograph, we improved the planets mass measurements in anticipation of Hubble Space Telescope transmission spectroscopy. For GJ9827, we modeled activity-induced radial velocity signals with a Gaussian process informed by the CalciumII H&amp;K lines in order to more accurately model the effect of stellar noise on our data. We measured planet masses of Mb=4.87{+/-}0.37M{Earth}, Mc=1.92{+/-}0.49M{Earth}, and Md=3.42{+/-}0.62M{Earth}. For HD 06315, we found that such activity radial velocity decorrelation was not effective due to the reduced presence of spots and speculate that this may extend to other hot stars as well (Teff&gt;6200K). We measured planet masses of Mb=10.5{+/-}3.1M{Earth} and Mc=12.0{+/-}3.8M{Earth}. We investigated all of the planets compositions through comparison of their masses and radii to a range of interior models. GJ9827b and GJ9827c are both consistent with a 50/50 rock-iron composition, GJ9827d and HD106315b both require additional volatiles and are consistent with moderate amounts of water or hydrogen/helium, and HD106315c is consistent with a ~10% hydrogen/helium envelope surrounding an Earth-like rock and iron core.</description><source format="bibcode">2021AJ....161...47K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/47</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/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/725/875">J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/A75">J/A+A/529/A75 : Limb-darkening coefficients (Claret+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/19">J/AJ/142/19 : Speckle observations of KOI (Howell+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/3">J/ApJ/764/3 : H{alpha} indices in M low-mass stars (Robertson+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/805/175">J/ApJ/805/175 : Keck and APF radial velocities of HD7924 (Fulton+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/109">J/AJ/154/109 : California-Kepler Survey. III. Planet radii (Fulton+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/102">J/ApJ/844/102 : KIC star plxs from asteroseismology vs Gaia (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/603/L5">J/A+A/603/L5 : HD106315c I light curve (Lendl+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/107">J/AJ/154/107 : California-Kepler Survey. I. 1305 stars (Petigura+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/836/77">J/ApJ/836/77 : Library of high-S/N optical spectra FGKM stars (Yee+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/484/3731">J/MNRAS/484/3731 : GJ 9827 HARPS-N RV data (Rice+, 2019)</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/161/47</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/161/47</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/161/47</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/161/47</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/161/47</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/161/47</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><spectral>2.762881831355591e-19 3.3785437584409506e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/161/47/rv</name><description>Combined table from original tables</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>ID</name><description>Star identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>BJD</name><description>Barycentric Julian Date; TDB</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</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_RVel</name><description>Uncertainty in RVel</description><unit>m/s</unit><ucd>stat.error;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SHK</name><description>? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>Star identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>HJD</name><description>Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Rmag</name><description>Differential Cousins R band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>