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<ri:Resource created="2024-10-22T10:41:08Z" status="active" updated="2025-07-03T20:01:08Z" 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>RGB stars from the APO-K2 catalogue</title><shortName>J/A+A/690/A323</shortName><identifier>ivo://CDS.VizieR/J/A+A/690/A323</identifier><altIdentifier>doi:10.26093/cds/vizier.36900323</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Valle G.</name></creator><creator><name>Dell'Omodarme M.</name></creator><creator><name>Prada Moroni P.G.</name></creator><creator><name>Degl'Innocenti S.</name></creator><date role="Updated">2025-07-03T20:01:08Z</date><date role="Created">2024-10-22T10:41:08Z</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>infrared-sources</subject><subject>giant-stars</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>stellar-radii</subject><description>By adopting the recently empirically derived dependence of {alpha}-elements on [alpha/Fe] instead of the conventionally applied uniform one, we tested the agreement between stellar model predictions and observations for RGB stars in the APO-K2 catalogue. We particularly focused on the biases in effective temperature scales and on the robustness of age estimations. A slight {DELTA}T difference of 25K was detected between stars with high and low {alpha}-enhancement. A multivariate analysis reveals a dependence of {DELTA}T on both [Fe/H] and [{alpha}/Fe], and highlights a significant dependence on stellar mass. Despite differences in assumed chemical composition, our analysis, through a fortunate cancellation effect, yields ages that are largely consistent with recent studies of the same sample. Notably, our analysis identifies a 6% fraction of stars younger than 4 Ga within the high-{alpha} population. However, our analysis of the [C/N] ratio supports the possible origin of the these stars as a result of mergers or mass transfer events.</description><source format="bibcode">2024A&amp;A...690A.323V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/690/A323</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/167/50">J/AJ/167/50 : The APO-K2 Catalog. 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