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<ri:Resource created="2006-12-17T21:58:58Z" 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>Carbon abundances in metal-poor stars</title><shortName>J/AJ/130/2804</shortName><identifier>ivo://CDS.VizieR/J/AJ/130/2804</identifier><altIdentifier>doi:10.26093/cds/vizier.51302804</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rossi S.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Sneden C.</name></creator><creator><name>Sevastyanenko T.</name></creator><creator><name>Rhee J.</name></creator><creator><name>Marsteller B.</name></creator><date role="Updated">2017-12-12T14:45:18Z</date><date role="Created">2006-12-17T21:58:58Z</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>chemical-abundances</subject><subject>carbon-stars</subject><subject>chemically-peculiar-stars</subject><description>We develop and test a method for the estimation of metallicities ([Fe/H]) and carbon abundance ratios ([C/Fe]) for carbon-enhanced metal-poor (CEMP) stars based on the application of artificial neural networks, regressions, and synthesis models to medium-resolution (1-2{AA}) spectra and J-K colors. We calibrate this method by comparison with metallicities and carbon abundance determinations for 118 stars with available high-resolution analyses reported in the recent literature.</description><source format="bibcode">2005AJ....130.2804R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/130/2804</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/J/AJ/103/1987">J/AJ/103/1987 : Stars of very low metal abundance (Beers+ 1992)</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/A+A/356/238">J/A+A/356/238 : Atmospheric parameters in metal-poor stars. 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