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<ri:Resource created="2021-07-15T09:16:45Z" 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>Catalog of gyro-kinematic ages for ~30000 Kepler stars</title><shortName>J/AJ/161/189</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/189</identifier><altIdentifier>doi:10.26093/cds/vizier.51610189</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lu Y.</name></creator><creator><name>Angus R.</name></creator><creator><name>Curtis J.L.</name></creator><creator><name>David T.J.</name></creator><creator><name>Kiman R.</name></creator><date role="Updated">2022-10-27T11:28:34Z</date><date role="Created">2021-07-15T09:16:45Z</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>stellar-ages</subject><subject>effective-temperature</subject><subject>dwarf-stars</subject><subject>visible-astronomy</subject><description>Estimating stellar ages is important for advancing our understanding of stellar and exoplanet evolution and investigating the history of the Milky Way. However, ages for low-mass stars are hard to infer as they evolve slowly on the main sequence. In addition, empirical dating methods are difficult to calibrate for low-mass stars as they are faint. In this work, we calculate ages for Kepler F, G, and crucially K and M-dwarfs, using their rotation and kinematic properties. We apply the simple assumption that the velocity dispersion of stars increases over time and adopt an age-velocity-dispersion relation (AVR) to estimate average stellar ages for groupings of coeval stars. We calculate the vertical velocity dispersion of stars in bins of absolute magnitude, temperature, rotation period, and Rossby number and then convert velocity dispersion to kinematic age via an AVR. Using this method, we estimate gyro-kinematic ages for 29949 Kepler stars with measured rotation periods. We are able to estimate ages for clusters and asteroseismic stars with an rms of 1.22Gyr and 0.26Gyr respectively. With our Astraea machine-learning algorithm, which predicts rotation periods, we suggest a new selection criterion (a weight of 0.15) to increase the size of the McQuillan et al. catalog of Kepler rotation periods by up to 25%. Using predicted rotation periods, we estimated gyro-kinematic ages for stars without measured rotation periods and found promising results by comparing 12 detailed age-element abundance trends with literature values.</description><source format="bibcode">2021AJ....161..189L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/189</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/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</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/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/695/679">J/ApJ/695/679 : Stellar rotation in M35 (Meibom+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/L9">J/ApJ/733/L9 : Stellar rotation for 71 NGC 6811 members (Meibom+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/48">J/ApJ/743/48 : Stars with rotation periods &amp; X-ray luminosities (Wright+,2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/776/67">J/ApJ/776/67 : Rotational tracks (van Saders+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/572/A34">J/A+A/572/A34 : Pulsating solar-like stars in Kepler (Garcia+, 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/AJ/152/113">J/AJ/152/113 : Pleiades members with K2 lightcurves.I. 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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>Target identification number, Kepler Input Catalog (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Prot</name><description>[0.2/68] Rotation period (2)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Prot</name><description>[0/10] Error on rotation period (2)</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RA_ICRS</name><description>[279/302] Right Ascension, Gaia DR2 (ICRS) at Ep=2015.5</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>e_RA_ICRS</name><description>[0.009/0.62] Error on RAdeg from Gaia DR2 (3)</description><unit>deg</unit><ucd>stat.error;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DE_ICRS</name><description>[36.5/52.5] Declination, Gaia DR2 (ICRS) at Ep=2015.5 (3)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>e_DE_ICRS</name><description>[0.01/0.7] Arror on DEdeg from Gaia DR2 (3)</description><unit>deg</unit><ucd>stat.error;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Wvel</name><description>[-259/415] Vertical velocity (4)</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Wvel</name><description>[0.03/42]? Error on Wvel (4)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sigma</name><description>[0.10/137] Velocity dispersion (5)</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_sigma</name><description>[0/0.07] Error on sigma (5)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GyroAge</name><description>[0.002/142] Gyro-kinematic ages (6)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_GyroAge</name><description>[1.6/2] Error on GyroAge (6)</description><unit>Gyr</unit><ucd>stat.error</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.icrs</name><description>Right ascension (ICRS) at Epoch=J2015.5 (computed by VizieR, not part of the original data. 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