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V.</title><shortName>J/ApJ/670/346</shortName><identifier>ivo://CDS.VizieR/J/ApJ/670/346</identifier><altIdentifier>doi:10.26093/cds/vizier.16700346</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chou M.-Y.</name></creator><creator><name>Majewski S.R.</name></creator><creator><name>Cunha K.</name></creator><creator><name>Smith V.V.</name></creator><creator><name>Patterson R.J.,Martinez-Delgado D.</name></creator><creator><name>Law D.R.</name></creator><creator><name>Crane J.D.</name></creator><creator><name>Munoz R.R.</name></creator><creator><name>Garcia Lopez R.,Geisler D.</name></creator><creator><name>Skrutskie M.F.</name></creator><date role="Updated">2018-07-04T12:06:59Z</date><date role="Created">2010-03-11T15:21:00Z</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>m-stars</subject><subject>spectroscopy</subject><subject>line-intensities</subject><description>We present reliable measurements of the metallicity distribution function (MDF) at different points along the tidal stream of the Sagittarius (Sgr) dwarf spheroidal (dSph) galaxy, based on high-resolution, echelle spectroscopy of candidate M giant members of the Sgr system.</description><source format="bibcode">2007ApJ...670..346C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/670/346</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 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