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<ri:Resource created="2020-09-28T14:22:05Z" 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>Gaia and LAMOST DR4 M giant members of Sgr stream</title><shortName>J/ApJ/874/138</shortName><identifier>ivo://CDS.VizieR/J/ApJ/874/138</identifier><altIdentifier>doi:10.26093/cds/vizier.18740138</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li J.</name></creator><creator><name>Liu C.</name></creator><creator><name>Xue X.</name></creator><creator><name>Zhong J.</name></creator><creator><name>Weiss J.</name></creator><creator><name>Carlin J.L.</name></creator><creator><name>Tian H.</name></creator><date role="Updated">2021-08-11T12:05:26Z</date><date role="Created">2020-09-28T14:22:05Z</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>m-stars</subject><subject>giant-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><subject>infrared-photometry</subject><subject>stellar-distance</subject><subject>metallicity</subject><subject>proper-motions</subject><description>We use LAMOST DR4 M giants combined with Gaia DR2 proper motions and ALLWISE photometry to obtain an extremely pure sample of Sagittarius (Sgr) stream stars. Using TiO5 and CaH spectral indices as indicators, we selected a large sample of M-giant stars from M-dwarf stars in LAMOST DR4 spectra. Considering the position, distance, proper motion, and angular momentum distribution, we obtained 164 pure Sgr stream stars. We find that the trailing arm has higher energy than the leading arm in the same angular momentum. The trailing arm we detected extends to a heliocentric distance of ~130kpc at {Lambda}_{sun}_~170{deg}, which is consistent with the feature found in RR Lyrae in Sesar+ (2017, J/ApJ/844/L4). Both of these detections of Sgr, in M-giants and in RR Lyrae, imply that the Sgr stream may contain multiple stellar populations with a broad metallicity range.</description><source format="bibcode">2019ApJ...874..138L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/874/138</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/198">III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/153">V/153 : LAMOST DR4 catalogs (Luo+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/113/806">J/AJ/113/806 : M-Subdwarfs (Gizis 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/508/397">J/ApJ/508/397 : H-band Spectral Standards (Meyer+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/1598">J/AJ/125/1598 : New high PM stars in the northern sky (Lepine+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/670/346">J/ApJ/670/346 : M giant stars in the Sagittarius dwarf galaxy. V. (Chou+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/90">J/ApJ/753/90 : Stellar param. of K5 and later type Kepler stars (Mann+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/102">J/AJ/145/102 : Bright M dwarf spectroscopy in the northern sky (Lepine+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/440/3430">J/MNRAS/440/3430 : SDSS-2MASS-WISE stellar colour locus (Davenport+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RAA/15.1154">J/other/RAA/15.1154 : M-giant star candidates in LAMOST DR 1 (Zhong+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/226/1">J/ApJS/226/1 : Carbon stars from LAMOST DR2 data (Ji+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/823/59">J/ApJ/823/59 : WISE and 2MASS photometry of M giant stars (Li+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/844/L4">J/ApJ/844/L4 : PS1 RRab 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