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<ri:Resource created="2017-12-05T06:26:57Z" 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>Constraining cosmic scatter</title><shortName>J/A+A/608/A46</shortName><identifier>ivo://CDS.VizieR/J/A+A/608/A46</identifier><altIdentifier>doi:10.26093/cds/vizier.36080046</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Reggiani H.</name></creator><creator><name>Melendez J.</name></creator><creator><name>Kobayashi C.</name></creator><creator><name>Karakas A.</name></creator><creator><name>Placco V.</name></creator><date role="Updated">2017-12-13T19:29:59Z</date><date role="Created">2017-12-05T06:26:57Z</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>population-ii-stars</subject><subject>metallicity</subject><subject>spectroscopy</subject><description>We present the stellar parameters, abundances, associated errors and the linelist of a set of 23 metal-poor and very metal-poor halo stars. Stellar parameters and chemical abundances were derived in a line-by-line differential analysis from equivalent widths of UVES/VLT spectra. The differential analysis provided us unprecedented small data scatter and errors. 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