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<ri:Resource created="2008-06-07T17:18:12Z" 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>CaII triplet of RGB from VLT/FLAMES obs.</title><shortName>J/MNRAS/383/183</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/383/183</identifier><altIdentifier>doi:10.26093/cds/vizier.73830183</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Battaglia G.</name></creator><creator><name>Irwin M.</name></creator><creator><name>Tolstoy E.</name></creator><creator><name>Hill V.</name></creator><creator><name>Helmi A.</name></creator><creator><name>Letarte B.,Jablonka P.</name></creator><date role="Updated">2024-07-05T20:16:04Z</date><date role="Created">2008-06-07T17:18:12Z</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>galaxies</subject><subject>globular-star-clusters</subject><subject>giant-stars</subject><subject>spectroscopy</subject><description>We demonstrate that low-resolution CaII triplet (CaT) spectroscopic estimates of the overall metallicity ([Fe/H]) of individual red giant branch (RGB) stars in two nearby dwarf spheroidal galaxies (dSphs) agree to +/-0.1-0.2dex with detailed high-resolution spectroscopic determinations for the same stars over the range -2.5&lt;[Fe/H]&lt;-0.5. For this study, we used a sample of 129 stars observed in low- and high-resolution modes with VLT/FLAMES in the Sculptor and Fornax dSphs. We also present the data-reduction steps we used in our low-resolution analysis and show that the typical accuracy of our velocity and CaT [Fe/H] measurement is ~2km/s and 0.1dex, respectively. We conclude that CaT[Fe/H] relations calibrated on globular clusters can be applied with confidence to RGB stars in composite stellar populations over the range -2.5&lt;[Fe/H]&lt;-0.5.</description><source format="bibcode">2008MNRAS.383..183B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/383/183</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/MNRAS/327/918">J/MNRAS/327/918 : CaII in extragalactic red giants (Tolstoy+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/459/423">J/A+A/459/423 : VI and [Fe/H] of Fornax dSph RGB 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