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<ri:Resource created="2021-04-28T07:51:37Z" 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>Ages and alpha-abundances of population in K2</title><shortName>J/AJ/161/100</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/100</identifier><altIdentifier>doi:10.26093/cds/vizier.51610100</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Warfield J.T.</name></creator><creator><name>Zinn J.C.</name></creator><creator><name>Pinsonneault M.H.</name></creator><creator><name>Johnson J.A.</name></creator><creator><name>Stello D.,Elsworth Y.</name></creator><creator><name>Garcia R.A.</name></creator><creator><name>Kallinger T.</name></creator><creator><name>Mathur S.</name></creator><creator><name>Mosser B.</name></creator><creator><name>Beaton R.L.,Garcia-Hernandez D.A.</name></creator><date role="Updated">2023-05-12T11:22:21Z</date><date role="Created">2021-04-28T07:51:37Z</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>surveys</subject><subject>milky-way-galaxy</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><subject>giant-stars</subject><subject>chemical-abundances</subject><subject>effective-temperature</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>We explore the relationships between the chemistry, ages, and locations of stars in the Galaxy using asteroseismic data from the K2 mission and spectroscopic data from the Apache Point Galactic Evolution Experiment survey. Previous studies have used giant stars in the Kepler field to map the relationship between the chemical composition and the ages of stars at the solar circle. Consistent with prior work, we find that stars with high [{alpha}/Fe] have distinct, older ages in comparison to stars with low [{alpha}/Fe]. We provide age estimates for red giant branch (RGB) stars in the Kepler field, which support and build upon previous age estimates by taking into account the effect of {alpha}-enrichment on opacity. Including this effect for [{alpha}/Fe]-rich stars results in up to 10% older ages for low- mass stars relative to corrected solar mixture calculations. This is a significant effect that Galactic archeology studies should take into account. Looking beyond the Kepler field, we estimate ages for 735 RGB stars from the K2 mission, mapping age trends as a function of the line of sight. We find that the age distributions for low- and high-[{alpha}/Fe] stars converge with increasing distance from the Galactic plane, in agreement with suggestions from earlier work. We find that K2 stars with high [{alpha}/Fe] appear to be younger than their counterparts in the Kepler field, overlapping more significantly with a similarly aged low-[{alpha}/Fe] population. This observation may suggest that star formation or radial migration proceeds unevenly in the Galaxy.</description><source format="bibcode">2021AJ....161..100W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/100</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/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/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/410/527">J/A+A/410/527 : Abundances in the Galactic disk (Bensby+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/16">J/ApJ/746/16 : Modelling the convection zone (van Saders+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/19">J/ApJS/215/19 : APOKASC catalog of Kepler red giants (Pinsonneault+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/445/2758">J/MNRAS/445/2758 : KIC giants Bayesian dist. &amp; extinctions (Rodrigues+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/2127">J/MNRAS/452/2127 : Fundamental parameters of Kepler stars (Silva Aguirre+,2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for 15 APOGEE chemic. elements (Garcia+,2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/597/A30">J/A+A/597/A30 : Seismology &amp; spectroscopy of CoRoGEE red giants (Anders+,2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/102">J/ApJ/844/102 : KIC star plxs from asteroseismology vs Gaia (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/173">J/ApJ/835/173 : Kepler asteroseismic LEGACY sample. 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Campaign 1 (Stello+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/32">J/ApJS/239/32 : APOKASC-2 catalog of Kepler evolved stars (Pinsonneault+,2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/18">J/AJ/156/18 : APOGEE DR14:Binary comp. of evolved stars (Price-Whelan+,2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/627/A173">J/A+A/627/A173 : Abundances for 4 metal-poor stars (Valentini+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/251/23">J/ApJS/251/23 : K2 GAP DR2: campaigns 4, 6 &amp; 7 (Zinn+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/645/A85">J/A+A/645/A85 : Age dissection of the Milky Way discs (Miglio+, 2021)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Corrected dnu from the A2Z pipeline from K2GAP</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_dnu.A2Z</name><description>[0.01/0.87]? Uncertainty on dnu.A2Z</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dnu.BAM</name><description>[1.24/14.4]? Corrected dnu from the BAM pipeline from K2GAP</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_dnu.BAM</name><description>[0.005/1.4]? Uncertainty on dnu.BAM</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dnu.CAN</name><description>[1.09/14]? Corrected dnu from the CAN pipeline from K2GAP</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logg.SEIS</name><description>[0.004/0.04] Uncertainty on logg.SEIS</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[0.3/3.67] Asteroseismic mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>[0.03/1.1]? Uncertainty on Mass</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>[0.33/11.4] Distance calculated from GAIA parallax from Bailer-Jones 2015</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Dist</name><description>[0.01/7.4] Uncertainty on Dist</description><unit>kpc</unit><ucd>stat.error;pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>X</name><description>[-12.3/-1.04] Galactocentric X coordinate calculated with astropy</description><unit>kpc</unit><ucd>pos.cartesian.x;pos.galactocentric;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>[-4.26/1.4] Galactocentric Y coordinate calculated with astropy</description><unit>kpc</unit><ucd>pos.cartesian.y;pos.galactocentric;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Z</name><description>[-2.37/8.66] Galactocentric Z coordinate calculated with astropy</description><unit>kpc</unit><ucd>pos.cartesian.z;pos.galactocentric;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R</name><description>[1.59/12.31] Galactocentric R coordinate calculated with astropy</description><unit>kpc</unit><ucd>pos.frame;pos.galactocentric;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/161/100/table4</name><description>RGB stars in the Kepler field, including our ages</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType><flag>nullable</flag></column><column><name>R</name><description>[7.73/11.09] Galactocentric R coordinate calculated with astropy</description><unit>kpc</unit><ucd>pos.frame;pos.galactocentric;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Position from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>KIC</name><description>MAST Kepler Input Catalog ID</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>APOGEE</name><description>APOGEE object ID</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>Age</name><description>[0.28/150] Median calculated stellar age</description><unit>Gyr</unit><ucd>time.age;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Age</name><description>[0.02/88] Lower 1-sigma deviation on Age</description><unit>Gyr</unit><ucd>stat.error;time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Age</name><description>[0.03/400] Upper 1-sigma deviation on Age</description><unit>Gyr</unit><ucd>stat.error;time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age.APO</name><description>[0.4/17.7] Calculated stellar age from Pinsonneault et al. 2018</description><unit>Gyr</unit><ucd>time.age;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[3942/5239] Corrected effective temperature from APOGEE DR16</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Teff</name><description>[65/130] Uncertainty on Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logg</name><description>[1.41/3.35] Corrected log surface gravity from APOGEE DR16</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logg</name><description>[0.02/0.12] Uncertainty on logg</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>[alpha/M]</name><description>[6e-06/0.39] Alpha abundance from APOGEE DR16</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[alpha/M]</name><description>[0.004/0.03] Uncertainty on [alpha/M]</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>[Fe/H]</name><description>[-2.15/0.45] Metallicity from APOGEE DR16</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_[Fe/H]</name><description>[0.005/0.03] Uncertainty on [Fe/H]</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>numax</name><description>[4.78/249] Mean value of numax from all pipelines from APOKASC2</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_numax</name><description>[0.05/7.01] Uncertainty on numax</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dnu</name><description>[0.74/19.2] Mean value of dnu from all pipelines from APOKASC2, with our f_dnu_ correction</description><unit>uHz</unit><ucd>em.freq;src.var</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dnu</name><description>[0.004/0.5] Uncertainty on dnu</description><unit>uHz</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[0.53/3.4] Asteroseismic mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>[0.03/1.1] Uncertainty on Mass</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>X</name><description>[-8.26/-5.69] Galactocentric X coordinate calculated with astropy</description><unit>kpc</unit><ucd>pos.cartesian.x;pos.galactocentric;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>[0.19/9.18] Galactocentric Y coordinate calculated with astropy</description><unit>kpc</unit><ucd>pos.cartesian.y;pos.galactocentric;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Z</name><description>[0.06/2.58] Galactocentric Z coordinate calculated with astropy</description><unit>kpc</unit><ucd>pos.cartesian.z;pos.galactocentric;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>