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<ri:Resource created="2012-08-17T16:13:31Z" 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>SEGUE stellar parameter pipeline. IV.</title><shortName>J/AJ/141/89</shortName><identifier>ivo://CDS.VizieR/J/AJ/141/89</identifier><altIdentifier>doi:10.26093/cds/vizier.51410089</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Smolinski J.P.</name></creator><creator><name>Lee Y.S.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>An D.</name></creator><creator><name>Bickerton S.J.</name></creator><creator><name>Johnson J.A.,Loomis C.P.</name></creator><creator><name>Rockosi C.M.</name></creator><creator><name>Sivarani T.</name></creator><creator><name>Yanny B.</name></creator><date role="Updated">2017-09-22T16:15:39Z</date><date role="Created">2012-08-17T16:13:31Z</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>globular-star-clusters</subject><subject>open-star-clusters</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><description>Spectroscopic and photometric data for likely member stars of five Galactic globular clusters (M3, M53, M71, M92, and NGC 5053) and three open clusters (M35, NGC 2158, and NGC 6791) are processed by the current version of the SEGUE Stellar Parameter Pipeline (SSPP), in order to determine estimates of metallicities and radial velocities (RVs) for the clusters. These results are then compared to values from the literature.</description><source format="bibcode">2011AJ....141...89S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/141/89</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/136/2050">J/AJ/136/2050 : SEGUE stellar parameter pipeline. II. (Lee+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2070">J/AJ/136/2070 : SEGUE stellar parameter pipeline. III. (Lee+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/90">J/AJ/141/90 : SEGUE stellar parameter pipeline. V. 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