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<ri:Resource created="2017-10-02T07:41:21Z" status="active" updated="2026-02-10T20:07:24Z" 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>K giant stars along Sagittarius streams</title><shortName>J/other/RAA/17.7</shortName><identifier>ivo://CDS.VizieR/J/other/RAA/17.76</identifier><altIdentifier>doi:10.26093/cds/vizier/dx/bhkhg</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ren H.-B.</name></creator><creator><name>Shi W.-B.</name></creator><creator><name>Zhang X.</name></creator><creator><name>Tang Y.-K.</name></creator><creator><name>Zhang Y.</name></creator><creator><name>Hou Y.-H.</name></creator><creator><name>Wang Y.-F.</name></creator><date role="Updated">2026-02-10T20:07:24Z</date><date role="Created">2017-10-02T07:41:21Z</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>milky-way-galaxy</subject><subject>giant-stars</subject><subject>k-stars</subject><subject>stellar-distance</subject><description>The Large Sky-Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 3 provided 341 691 K giant stars with stellar parameters. Based on the models of Law &amp; Majewski (2010ApJ...714..229L), we identified 252 K giant stars in the leading stream associated with the Sagittarius (Sgr) dwarf galaxy. We obtained 132 K giant stars belonging to the trailing arm of Sgr using the model of Belokurov et al. We studied the metallicity distribution of member stars along the streams and found a flat gradient in the first wrap of the leading stream, -(0.88+/-0.3)x10^-3^dex/deg in the second wrap of the leading stream and -(1.2+/-0.3)x10^-3^dex/deg in the first wrap of the trailing stream. Moreover, we obtained a combined metallicity gradient with our sample and data from the literature. 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