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<ri:Resource created="2015-02-18T08:33:45Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>Spectroscopy of faint KOI stars</title><shortName>J/ApJ/771/107</shortName><identifier>ivo://CDS.VizieR/J/ApJ/771/107</identifier><altIdentifier>doi:10.26093/cds/vizier.17710107</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Everett M.E.</name></creator><creator><name>Howell S.B.</name></creator><creator><name>Silva D.R.</name></creator><creator><name>Szkody P.</name></creator><date role="Updated">2017-12-22T05:32:11Z</date><date role="Created">2015-02-18T08:33:45Z</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>solar-system-planets</subject><subject>multiple-stars</subject><subject>stellar-radii</subject><subject>metallicity</subject><description>Stellar properties are measured for a large set of Kepler mission exoplanet candidate host stars. Most of these stars are fainter than 14th magnitude, in contrast to other spectroscopic follow-up studies. This sample includes many high-priority Earth-sized candidate planets. A set of model spectra are fitted to R~3000 optical spectra of 268 stars to improve estimates of T_eff_, log(g), and [Fe/H] for the dwarfs in the range 4750&lt;=T_eff_&lt;=7200K. These stellar properties are used to find new stellar radii and, in turn, new radius estimates for the candidate planets. The result of improved stellar characteristics is a more accurate representation of this Kepler exoplanet sample and identification of promising candidates for more detailed study. This stellar sample, particularly among stars with T_eff_&gt;~5200K, includes a greater number of relatively evolved stars with larger radii than assumed by the mission on the basis of multi-color broadband photometry. About 26% of the modeled stars require radii to be revised upward by a factor of 1.35 or greater, and modeling of 87% of the stars suggest some increase in radius. The sample presented here also exhibits a change in the incidence of planets larger than 3-4R_{Earth}_ as a function of metallicity. Once [Fe/H] increases to &gt;=-0.05, large planets suddenly appear in the sample while smaller planets are found orbiting stars with a wider range of metallicity.</description><source format="bibcode">2013ApJ...771..107E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/771/107</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/120">VI/120 : High-resolution synthetic stellar library (Coelho+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/5">J/ApJS/213/5 : Cool KOIs. VI. H- and K- band spectra (Muirhead+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/2">J/ApJS/211/2 : Revised properties of Q1-16 Kepler targets (Huber+, 2014)</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/ApJS/210/19">J/ApJS/210/19 : Kepler planetary candidates. IV. 22 months (Burke+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/1">J/ApJS/210/1 : Asteroseismic study of solar-type stars (Chaplin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/69">J/ApJ/770/69 : Kepler planet candidates radii (Petigura+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/43">J/ApJ/770/43 : Spectroscopic [Fe/H] of Kepler planet hosts (Mann+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/95">J/ApJ/767/95 : Improved stellar param. of KIC stars (Dressing+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/L37">J/ApJ/750/L37 : Stellar parameters of low-mass KOIs (Muirhead+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/30">J/ApJS/199/30 : Effective temperature for KIC stars (Pinsonneault+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/486.375">J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/423/122">J/MNRAS/423/122 : Abundances of 93 solar-type Kepler targets (Bruntt+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/112">J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/738/170">J/ApJ/738/170 : False positive Kepler planet candidates (Morton+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/704/1107">J/ApJ/704/1107 : Transiting planets in HATNet field 205 (Latham+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2464">J/AJ/133/2464 : Parameters and abundances of nearby giants (Luck+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/159/141">J/ApJS/159/141 : Spectroscopic properties of cool stars. 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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>KOI</name><description>Planet identifier (&lt;KOI-NNNN.NN&gt; in Simbad)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>KIC</name><description>Kepler parent star identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(Teff)</name><description>[3.6/3.9] Log of the effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(g)</name><description>[4/4.7] Log of the surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-0.3/0.3] Metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R*</name><description>[0.7/2] Stellar radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ratio</name><description>[0.5/2.2] Ratio of revised to KSAS derived stellar radii (1)</description><ucd>stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rp</name><description>[0.4/59] Planetary radius; Earth radii</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from Kepler Input Catalog (V/133) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from Kepler Input Catalog (V/133) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/771/107/table2</name><description>Stellar properties determined for 352 KOIs</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>KOI</name><description>[13/3259] Kepler Object of Interest number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>KIC</name><description>Kepler identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Np</name><description>Number of planet candidates in table 3</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Kpmag</name><description>[9.5/16.5] Observed Kepler magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[4750/6606]? 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