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<ri:Resource created="2018-11-06T07:41:26Z" 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>28 distant globular clusters CaT metallicities</title><shortName>J/A+A/619/A13</shortName><identifier>ivo://CDS.VizieR/J/A+A/619/A13</identifier><altIdentifier>doi:10.26093/cds/vizier.36190013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Vasquez S.</name></creator><creator><name>Saviane I.</name></creator><creator><name>Held E.V.</name></creator><creator><name>Da Costa G.S.</name></creator><creator><name>Dias B.</name></creator><creator><name>Gullieuszik M.,Barbuy B.</name></creator><creator><name>Ortolani S.</name></creator><creator><name>Zoccali M.</name></creator><date role="Updated">2018-12-03T15:09:40Z</date><date role="Created">2018-11-06T07:41:26Z</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>giant-stars</subject><subject>line-intensities</subject><subject>radial-velocity</subject><description>In an earlier paper we presented the first part of a project to obtain metallicities and radial velocities of Galactic globular clusters from multiobject spectroscopy of their member stars using the ESO Very Large Telescope. In this paper we add metallicities and radial velocities for a new sample of 28 globular clusters, including in particular globular clusters in the MW halo and the Galactic bulge. Together with our previous results, this study brings the number of globular clusters with homogeneous measurements to ~69% of those listed in the W. Harris' catalogue. As in our previous work, we have used the CaII triplet lines to derive metallicities and radial velocities. For most of the clusters in this study, this is the first analysis based on spectroscopy of individual member stars. 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