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<ri:Resource created="2006-10-07T21:13:39Z" 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>HERES II. Spectroscopic analysis</title><shortName>J/A+A/439/129</shortName><identifier>ivo://CDS.VizieR/J/A+A/439/129</identifier><altIdentifier>doi:10.26093/cds/vizier.34390129</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Barklem P.S.</name></creator><creator><name>Christlieb N.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Hill V.</name></creator><creator><name>Bessell M.S.</name></creator><creator><name>Holmberg J.,Marsteller B.</name></creator><creator><name>Rossi S.</name></creator><creator><name>Zickgraf F.-J.</name></creator><creator><name>Reimers D.</name></creator><date role="Updated">2017-06-26T11:49:04Z</date><date role="Created">2006-10-07T21:13:39Z</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>chemically-peculiar-stars</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><description>We present the results of analysis of "snapshot" spectra of 253 metal-poor halo stars -3.8&lt;=[Fe/H]&lt;=-1.5 obtained in the HERES survey. The snapshot spectra have been obtained with VLT/UVES and have typically S/N~54 per pixel (ranging from 17 to 308), R~20000, lambda=3760-4980{AA}. 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