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<ri:Resource created="2015-01-29T14:09:07Z" 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>Candidate planets in the habitable zones</title><shortName>J/ApJ/770/90</shortName><identifier>ivo://CDS.VizieR/J/ApJ/770/90</identifier><altIdentifier>doi:10.26093/cds/vizier.17700090</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gaidos E.</name></creator><date role="Updated">2017-09-19T14:24:11Z</date><date role="Created">2015-01-29T14:09:07Z</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-masses</subject><subject>stellar-ages</subject><subject>metallicity</subject><description>A key goal of the Kepler mission is the discovery of Earth-size transiting planets in "habitable zones" where stellar irradiance maintains a temperate climate on an Earth-like planet. Robust estimates of planet radius and irradiance require accurate stellar parameters, but most Kepler systems are faint, making spectroscopy difficult and prioritization of targets desirable. The parameters of 2035 host stars were estimated by Bayesian analysis and the probabilities p_HZ_ that 2738 candidate or confirmed planets orbit in the habitable zone were calculated. Dartmouth Stellar Evolution Program models were compared to photometry from the Kepler Input Catalog, priors for stellar mass, age, metallicity and distance, and planet transit duration. The analysis yielded probability density functions for calculating confidence intervals of planet radius and stellar irradiance, as well as p_HZ_. Sixty-two planets have p_HZ_&gt;0.5 and a most probable stellar irradiance within habitable zone limits. Fourteen of these have radii less than twice the Earth; the objects most resembling Earth in terms of radius and irradiance are KOIs 2626.01 and 3010.01, which orbit late K/M-type dwarf stars. The fraction of Kepler dwarf stars with Earth-size planets in the habitable zone ({eta}_{Earth}_) is 0.46, with a 95% confidence interval of 0.31-0.64. Parallaxes from the Gaia mission will reduce uncertainties by more than a factor of five and permit definitive assignments of transiting planets to the habitable zones of Kepler stars.</description><source format="bibcode">2013ApJ...770...90G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/770/90</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/V/136">V/136 : Teff and metallicities for Tycho-2 stars (Ammons+, 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/A+A/567/A133">J/A+A/567/A133 : Habitable zone code (Valle+, 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 param. of smallest KIC stars (Dressing+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/102">J/AJ/145/102 : Bright M dwarfs spectro. in the northern sky (Lepine+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/204/24">J/ApJS/204/24 : Kepler planetary candidates. III. (Batalha+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A109">J/A+A/549/A109 : HARPS XXXI. The M-dwarf sample (Bonfils+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/24">J/AJ/144/24 : The Kepler-INT survey (Greiss+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. II. K and M-stars (Boyajian+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/186">J/ApJ/756/186 : TTVs from Kepler. VI. Statistical tests (Steffen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/90">J/ApJ/753/90 : Stellar param. of K5 &amp; later type Kepler stars (Mann+, 2012)</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 : KIC stars effective temperature scale (Pinsonneault+, 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/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/411/435">J/MNRAS/411/435 : Stellar parameters and extinction (Bailer-Jones, 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/ApJ/736/19">J/ApJ/736/19 : Kepler planetary candidates. II. (Borucki+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/L25">J/ApJ/736/L25 : Habitability of Kepler planetary cand. 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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>f_KOI</name><description>[o] "o" for other HZ candidates (pHZ&lt;0.5) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>KOI</name><description>[87.01/3086.01] KOI planet candidate ID</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>KIC</name><description>[2973386/12417486] KIC star number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>pHZ</name><description>[0.03/1] Habitable Zone probability</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>[14.9/574] Orbital period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ir</name><description>[0.2/3.3] Most probable value of Irradiance; in I_{Earth}_ unit</description><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_Ir</name><description>[0.1/2] 95% lower limit on Ir</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_Ir</name><description>[0.2/25] 95% upper limit on Ir</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rp</name><description>[1/11.5] Most probable planet radius</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_Rp</name><description>[0.8/11] 95% lower limit on Rp</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_Rp</name><description>[1/27] 95% upper limit on Rp</description><unit>(6.3781x10+6m)</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[3542/6244] Star effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[4.2/5] Star surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phot.sb</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>[-0.5/0.2] Star metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L*</name><description>[0.01/2.1] Log of stellar luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M*</name><description>[0.3/1.2] Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age</name><description>[1/8.6] Stellar age</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kepler</name><description>Planet Kepler name</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Ref</name><description>Reference(s) (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType></column><column><name>M</name><description>Data from Buchhave et al. 2012, J/other/Nat/486.375; Muirhead et al. 2012, J/ApJ/750/L37; Borucki et al. 2011, J/ApJ/736/19; Kaltenegger et al. 2011, J/ApJ/736/L25; Batalha et al. 2013, J/ApJS/204/24; Dressing et al. 2013, J/ApJ/767/95</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></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></schema></tableset></ri:Resource>