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<ri:Resource created="2012-07-27T09:49:51Z" 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>Effective temperature scale for KIC stars</title><shortName>J/ApJS/199/30</shortName><identifier>ivo://CDS.VizieR/J/ApJS/199/30</identifier><altIdentifier>doi:10.26093/cds/vizier.21990030</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pinsonneault M.H.</name></creator><creator><name>An D.</name></creator><creator><name>Molenda-Zakowicz J.</name></creator><creator><name>Chaplin W.J.</name></creator><creator><name>Metcalfe T.S.,Bruntt H.</name></creator><date role="Updated">2017-12-12T14:44:31Z</date><date role="Created">2012-07-27T09:49:51Z</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>effective-temperature</subject><subject>metallicity</subject><subject>multiple-stars</subject><description>We present a catalog of revised effective temperatures for stars observed in long-cadence mode in the Kepler Input Catalog (KIC). We use Sloan Digital Sky Survey (SDSS) griz filters tied to the fundamental temperature scale. Polynomials for griz color-temperature relations are presented, along with correction terms for surface gravity effects, metallicity, and statistical corrections for binary companions or blending. We compare our temperature scale to the published infrared flux method (IRFM) scale for V_T_JKs in both open clusters and the Kepler fields. We find good agreement overall, with some deviations between (J-Ks)-based temperatures from the IRFM and both SDSS filter and other diagnostic IRFM color-temperature relationships above 6000K. For field dwarfs, we find a mean shift toward hotter temperatures relative to the KIC, of order 215K, in the regime where the IRFM scale is well defined (4000K to 6500K). This change is of comparable magnitude in both color systems and in spectroscopy for stars with T_eff_ below 6000K. Systematic differences between temperature estimators appear for hotter stars, and we define corrections to put the SDSS temperatures on the IRFM scale for them. When the theoretical dependence on gravity is accounted for, we find a similar temperature scale offset between the fundamental and KIC scales for giants. We demonstrate that statistical corrections to color-based temperatures from binaries are significant. Typical errors, mostly from uncertainties in extinction, are of order 100K.</description><source format="bibcode">2012ApJS..199...30P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/199/30</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/II/306">II/306 : The SDSS Photometric Catalog, Release 8 (Adelman-McCarthy+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A138">J/A+A/530/A138 : Geneva-Copenhagen survey re-analysis (Casagrande+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/412/1210">J/MNRAS/412/1210 : Kepler asteroseismic targets (Molenda-Zakowicz+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A54">J/A+A/512/A54 : Teff and Fbol from Infrared Flux Method (Casagrande+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/523">J/ApJ/700/523 : Galactic star clusters in SDSS. II. Colors. (An+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/546/1006">J/ApJ/546/1006 : VRI photometry of M35 (Barrado y Navascues+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/130/65">J/A+AS/130/65 : A standard stellar library. II. 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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>KIC</name><description>Unique KIC catalog identification</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>T</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Te(S)</name><description>? SDSS derived effective temperature (1)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Te(S)</name><description>? Total uncertainty in Te(S)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>E_Te(S)</name><description>? 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