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<ri:Resource created="2015-10-21T11:49:48Z" status="active" updated="2025-06-13T15:25:00Z" 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>Highly likely members of the Sgr stream</title><shortName>J/ApJ/805/189</shortName><identifier>ivo://CDS.VizieR/J/ApJ/805/189</identifier><altIdentifier>doi:10.26093/cds/vizier.18050189</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hyde E.A.</name></creator><creator><name>Keller S.</name></creator><creator><name>Zucker D.B.</name></creator><creator><name>Ibata R.</name></creator><creator><name>Siebert A.</name></creator><creator><name>Lewis G.F.,Penarrubia J.</name></creator><creator><name>Irwin M.</name></creator><creator><name>Gilmore G.</name></creator><creator><name>Lane R.R.</name></creator><creator><name>Koch A.</name></creator><creator><name>Conn A.R.,Diakogiannis F.I.</name></creator><creator><name>Martell S.</name></creator><date role="Updated">2017-12-15T10:55:09Z</date><date role="Created">2015-10-21T11:49:48Z</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>chemical-abundances</subject><subject>halo-stars</subject><description>Wrapping around the Milky Way, the Sagittarius stream is the dominant substructure in the halo. Our statistical selection method has allowed us to identify 106 highly likely members of the Sagittarius stream. Spectroscopic analysis of metallicity and kinematics of all members provides us with a new mapping of the Sagittarius stream. We find correspondence between the velocity distribution of stream stars and those computed for a triaxial model of the Milky Way dark matter halo. The Sagittarius trailing arm exhibits a metallicity gradient, ranging from -0.59 to -0.97dex over 142{deg}. This is consistent with the scenario of tidal disruption from a progenitor dwarf galaxy that possessed an internal metallicity gradient. We note high metallicity dispersion in the leading arm, causing a lack of detectable gradient and possibly indicating orbital phase mixing. We additionally report on a potential detection of the Sextans dwarf spheroidal in our data.</description><source format="bibcode">2015ApJ...805..189H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/805/189</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/III/272">III/272 : RAVE 4th data release (Kordopatis+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/265">III/265 : RAVE 3rd data release (Siebert+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/317">I/317 : The PPMXL Catalog (Roeser+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/163">J/AJ/145/163 : Catalog of stars in Sgr dwarf galaxy (Newby+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/751/130">J/ApJ/751/130 : SDSS-DR7 red HB stars spectroscopic data (Shi+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/119">J/ApJ/731/119 : BHB candidates in Sagittarius stream (Ruhland+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/1290">J/ApJ/708/1290 : A 2MASS view of the Sgr dSph. 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(Chou+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/464/201">J/A+A/464/201 : RGB stars in Sagittarius streams (Monaco+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/245">J/AJ/128/245 : M giant stars in the Sgr dwarf galaxy (Majewski+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/2031">J/AJ/127/2031 : Catalog of neighboring galaxies (Karachentsev+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/414/503">J/A+A/414/503 : Abundances in the Sgr dSph (Bonifacio+, 2004)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/805/189</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/805/189</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/805/189</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/805/189</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/805/189</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/805/189</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/805/189/table2 (The selected 106 likely Sagittarius Stream members with modified RAVE pipeline metallicity, surface gravity, and effective temperature values)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/805/189/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/805/189/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/805/189/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>29.5224167</ra><dec>-1.7531111</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/48 49 51 54 275 276 278 279 4449 6261 17797 17799 17808 17810 23928 23930 24219 24222 24244 25917 25918 25919 25962 27207 27218 27224 28093 28136 28138 28203 28206 29337 30884 31397 44502 45001 45004 47014 47599 47940 47941</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/805/189?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/805/189/table2</name><description>The selected 106 likely Sagittarius Stream members with modified RAVE pipeline metallicity, surface gravity, and effective temperature values</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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