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<ri:Resource created="2011-09-27T12:12:16Z" 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>Astrometric Grid Giant Star Survey. I.</title><shortName>J/AJ/131/1784</shortName><identifier>ivo://CDS.VizieR/J/AJ/131/1784</identifier><altIdentifier>doi:10.26093/cds/vizier.51311784</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bizyaev D.</name></creator><creator><name>Smith V.V.</name></creator><creator><name>Arenas J.</name></creator><creator><name>Geisler D.</name></creator><creator><name>Majewski S.R.,Patterson R.J.</name></creator><creator><name>Cunha K.</name></creator><creator><name>Del Pardo C.</name></creator><creator><name>Suntzeff N.B.</name></creator><creator><name>Gieren W.</name></creator><date role="Updated">2017-12-22T05:33:32Z</date><date role="Created">2011-09-27T12:12:16Z</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>giant-stars</subject><subject>radial-velocity</subject><subject>metallicity</subject><description>We present results from a campaign of multiple-epoch echelle spectroscopy of relatively faint (V=9.5-13.5mag) red giants observed as potential astrometric grid stars for the Space Interferometry Mission (SIM PlanetQuest). Data are analyzed for 775 stars selected from the Grid Giant Star Survey, spanning a wide range of effective temperatures (Teff), gravities, and metallicities. 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