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<ri:Resource created="2020-11-05T13:49:57Z" 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>Gaia-Kepler stellar properties catalog. II. Planets</title><shortName>J/AJ/160/108</shortName><identifier>ivo://CDS.VizieR/J/AJ/160/108</identifier><altIdentifier>doi:10.26093/cds/vizier.51600108</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Berger T.A.</name></creator><creator><name>Huber D.</name></creator><creator><name>Gaidos E.</name></creator><creator><name>van Saders J.L.</name></creator><creator><name>Weiss L.M.</name></creator><date role="Updated">2022-06-03T06:10:45Z</date><date role="Created">2020-11-05T13:49:57Z</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>giant-stars</subject><subject>infrared-astronomy</subject><subject>visible-astronomy</subject><description>Studies of exoplanet demographics require large samples and precise constraints on exoplanet host stars. Using the homogeneous Kepler stellar properties derived using the Gaia Data Release 2 by Berger et al., we recompute Kepler planet radii and incident fluxes and investigate their distributions with stellar mass and age. We measure the stellar mass dependence of the planet radius valley to be dlogR_p/d_logM_{star}_=0.26_-0.16_^+0.21^, consistent with the slope predicted by a planet mass dependence on stellar mass (0.24-0.35) and core-powered mass loss (0.33). We also find the first evidence of a stellar age dependence of the planet populations straddling the radius valley. Specifically, we determine that the fraction of super-Earths (1-1.8{R_{Earth}_) to sub-Neptunes (1.8-3.5R_{Earth}_) increases from 0.61{+/-}0.09 at young ages (&lt;1Gyr) to 1.00{+/-}0.10 at old ages (&gt;1Gyr), consistent with the prediction by core-powered mass loss that the mechanism shaping the radius valley operates over Gyr timescales. Additionally, we find a tentative decrease in the radii of relatively cool (Fp&lt;150{F}_{Earth}_) sub-Neptunes over Gyr timescales, which suggests that these planets may possess H/He envelopes instead of higher mean molecular weight atmospheres. We confirm the existence of planets within the hot sub-Neptunian "desert" (2.2R_{Earth}_&lt;Rp&lt;3.8R_{Earth}_, Fp&gt;650F_{Earth}_) and show that these planets are preferentially orbiting more evolved stars compared to other planets at similar incident fluxes. In addition, we identify candidates for cool (Fp&lt;20F_{Earth}_) inflated Jupiters, present a revised list of habitable zone candidates, and find that the ages of single and multiple transiting planet systems are statistically indistinguishable.</description><source format="bibcode">2020AJ....160..108B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/160/108</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/1">J/ApJS/190/1 : A survey of stellar families (Raghavan+, 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/PASP/124/1279">J/PASP/124/1279 : Q3 Kepler's combined photometry (Christiansen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/771/107">J/ApJ/771/107 : Spectroscopy of faint KOI stars (Everett+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/775/L11">J/ApJ/775/L11 : Stellar rotation periods for KOIs (McQuillan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/780/159">J/ApJ/780/159 : Rotation-mass-age relation. old field stars (Epstein+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/790/146">J/ApJ/790/146 : Planets Kepler's multi-transiting systems (Fabrycky+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/2">J/ApJS/211/2 : Stellar properties of Q1-16 Kepler targets (Huber+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/791/35">J/ApJ/791/35 : Detection of 715 Kepler planet cand. host stars (Law+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/24">J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/801/3">J/ApJ/801/3 : Rotation periods for Q3-Q14 KOIs (Mazeh+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/813/100">J/ApJ/813/100 : Deep GALEX NUV survey of the Kepler field. 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