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<ri:Resource created="2014-09-15T14:24:23Z" 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>Cool KOIs. VI. H- and K- band spectra</title><shortName>J/ApJS/213/5</shortName><identifier>ivo://CDS.VizieR/J/ApJS/213/5</identifier><altIdentifier>doi:10.26093/cds/vizier.22130005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Muirhead P.S.</name></creator><creator><name>Becker J.</name></creator><creator><name>Feiden G.A.</name></creator><creator><name>Rojas-Ayala B.</name></creator><creator><name>Vanderburg A.,Price E.M.</name></creator><creator><name>Thorp R.</name></creator><creator><name>Law N.M.</name></creator><creator><name>Riddle R.</name></creator><creator><name>Baranec C.</name></creator><creator><name>Hamren K.,Schlawin E.</name></creator><creator><name>Covey K.R.</name></creator><creator><name>Johnson J.A.</name></creator><creator><name>Lloyd J.P.</name></creator><date role="Updated">2018-01-11T07:21:38Z</date><date role="Created">2014-09-15T14:24:23Z</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>multiple-stars</subject><subject>metallicity</subject><subject>stellar-spectral-types</subject><subject>stellar-masses</subject><subject>stellar-distance</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>solar-system-planets</subject><description>We present H- and K-band spectra for late-type Kepler Objects of Interest (the "Cool KOIs"): low-mass stars with transiting-planet candidates discovered by NASA's Kepler Mission that are listed on the NASA Exoplanet Archive. We acquired spectra of 103 Cool KOIs and used the indices and calibrations of Rojas-Ayala et al. (2012, Cat. J/ApJ/748/93) to determine their spectral types, stellar effective temperatures, and metallicities, significantly augmenting previously published values. We interpolate our measured effective temperatures and metallicities onto evolutionary isochrones to determine stellar masses, radii, luminosities, and distances, assuming the stars have settled onto the main sequence. As a choice of isochrones, we use a new suite of Dartmouth predictions that reliably include mid-to-late M dwarf stars. We identify five M4V stars: KOI-961 (confirmed as Kepler 42), KOI-2704, KOI-2842, KOI-4290, and the secondary component to visual binary KOI-1725, which we call KOI-1725B. We also identify a peculiar star, KOI-3497, which has Na and Ca lines consistent with a dwarf star but CO lines consistent with a giant. Visible-wavelength adaptive optics imaging reveals two objects within a 1 arcsec diameter; however, the objects' colors are peculiar. The spectra and properties presented in this paper serve as a resource for prioritizing follow-up observations and planet validation efforts for the Cool KOIs.</description><source format="bibcode">2014ApJS..213....5M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/213/5</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/I/322">I/322 : UCAC4 Catalogue (Zacharias+, 2012)</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</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/207/35">J/ApJS/207/35 : Kepler pipeline signal-to-noise studies (Christiansen+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/204/24">J/ApJS/204/24 : Kepler planetary candidates. 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(Borucki+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/117">J/ApJ/728/117 : Kepler planetary candidates. I. (Borucki+, 2011)</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/other/A+ARV/18.67">J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/159/141">J/ApJS/159/141 : Spectroscopic properties of cool stars. I. 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