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<ri:Resource created="2022-09-30T07:21:16Z" 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>Open cluster chemical abund. &amp; mapping survey. VII.</title><shortName>J/AJ/163/229</shortName><identifier>ivo://CDS.VizieR/J/AJ/163/229</identifier><altIdentifier>doi:10.26093/cds/vizier.51630229</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Spoo T.</name></creator><creator><name>Tayar J.</name></creator><creator><name>Frinchaboy P.M.</name></creator><creator><name>Cunha K.</name></creator><creator><name>Myers N.</name></creator><creator><name>Donor J.,Majewski S.R.</name></creator><creator><name>Bizyaev D.</name></creator><creator><name>Garcia-Hernandez D.A.</name></creator><creator><name>Jonsson H.</name></creator><creator><name>Lane R.R.,Pan K.</name></creator><creator><name>Longa-Pena P.</name></creator><creator><name>Roman-Lopes A.</name></creator><date role="Updated">2022-10-12T12:16:14Z</date><date role="Created">2022-09-30T07:21:16Z</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>open-star-clusters</subject><subject>giant-stars</subject><subject>chemical-abundances</subject><subject>metallicity</subject><subject>effective-temperature</subject><subject>infrared-astronomy</subject><description>Large-scale surveys open the possibility to investigate Galactic evolution both chemically and kinematically; however, reliable stellar ages remain a major challenge. Detailed chemical information provided by high-resolution spectroscopic surveys of the stars in clusters can be used as a means to calibrate recently developed chemical tools for age-dating field stars. Using data from the Open Cluster Abundances and Mapping survey, based on the Sloan Digital Sky Survey/Apache Point Observatory Galactic Evolution Experiment 2 survey, we derive a new empirical relationship between open cluster stellar ages and the carbon-to-nitrogen ([C/N]) abundance ratios for evolved stars, primarily those on the red giant branch. With this calibration, [C/N] can be used as a chemical clock for evolved field stars to investigate the formation and evolution of different parts of our Galaxy. We explore how mixing effects at different stellar evolutionary phases, like the red clump, affect the derived calibration. We have established the [C/N]-age calibration for APOGEE Data Release 17 (DR17) giant star abundances to be log[Age(yr)]_DR17_=10.14{+/-}0.08+2.23{+/-}0.19[C/N], usable for 8.62&lt;=log[Age(yr)]&lt;=9.82, derived from a uniform sample of 49 clusters observed as part of APOGEE DR17 applicable primarily to metal-rich, thin- and thick-disk giant stars. This measured [C/N]-age APOGEE DR17 calibration is also shown to be consistent with asteroseismic ages derived from Kepler photometry.</description><source format="bibcode">2022AJ....163..229S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/163/229</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/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/354/169">J/A+A/354/169 : Metal-poor field stars abundances (Gratton+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/221/24">J/ApJS/221/24 : SDSS-III APOGEE H-band spectral line lists (Shetrone+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for 15 APOGEE chemical elements (Garcia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/832/121">J/ApJ/832/121 : 4yr RV survey red giant in eclipsing binaries (Gaulme+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/456/3655">J/MNRAS/456/3655 : Masses and ages of red giants (Martig+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/823/114">J/ApJ/823/114 : The Cannon; a new approach to determine masses (Ness+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/102">J/ApJ/844/102 : KIC star parallaxe from asteroseismology vs Gaia (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/465/3203">J/MNRAS/465/3203 : GALAH observational overview (Martell+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/142">J/AJ/156/142 : Precision cluster abund. 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