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<ri:Resource created="2020-12-03T09:28:03Z" 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>Chemical abundances in red giants with Magellan</title><shortName>J/AJ/160/181</shortName><identifier>ivo://CDS.VizieR/J/AJ/160/181</identifier><altIdentifier>doi:10.26093/cds/vizier.51600181</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ji A.P.</name></creator><creator><name>Li T.S.</name></creator><creator><name>Hansen T.T.</name></creator><creator><name>Casey A.R.</name></creator><creator><name>Koposov S.E.</name></creator><creator><name>Pace A.B.,Mackey D.</name></creator><creator><name>Lewis G.F.</name></creator><creator><name>Simpson J.D.</name></creator><creator><name>Bland-Hawthorn J.</name></creator><creator><name>Cullinane L.R.,Da Costa G.S.</name></creator><creator><name>Hattori K.</name></creator><creator><name>Martell S.L.</name></creator><creator><name>Kuehn K.</name></creator><creator><name>Erkal D.</name></creator><creator><name>Shipp N.,Wan Z.</name></creator><creator><name>Zucker D.B.</name></creator><date role="Updated">2022-06-03T06:14:14Z</date><date role="Created">2020-12-03T09:28:03Z</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>chemical-abundances</subject><subject>effective-temperature</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We present high-resolution Magellan/MIKE spectroscopy of 42 red giant stars in seven stellar streams confirmed by the Southern Stellar Stream Spectroscopic Survey (S5): ATLAS, Aliqa Uma, Chenab, Elqui, Indus, Jhelum, and Phoenix. Abundances of 30 elements have been derived from over 10000 individual line measurements or upper limits using photometric stellar parameters and a standard LTE analysis. This is currently the most extensive set of element abundances for stars in stellar streams. Three streams (ATLAS, Aliqa Uma, and Phoenix) are disrupted metal-poor globular clusters, although only weak evidence is seen for the light-element anticorrelations commonly observed in globular clusters. Four streams (Chenab, Elqui, Indus, and Jhelum) are disrupted dwarf galaxies, and their stars display abundance signatures that suggest progenitors with stellar masses ranging from 106 to 107M{sun}. Extensive description is provided for the analysis methods, including the derivation of a new method for including the effect of stellar parameter correlations on each star's abundance and uncertainty. This paper includes data gathered with the 6.5m Magellan Telescopes located at Las Campanas Observatory, Chile.</description><source format="bibcode">2020AJ....160..181J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/160/181</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/B/simbad">B/simbad : Simbad objects catalogue (M.Wenger 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/357">II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/120/1841">J/AJ/120/1841 : Abundances &amp; Kinematics Halo &amp; Disk Stars (Fulbright, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/612/447">J/ApJ/612/447 : Draco 119 and HD 88609 equivalent widths (Fulbright+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/617/1091">J/ApJ/617/1091 : La and Eu abundances in 85 stars (Simmerer+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1177">J/AJ/128/1177 : Galactic stellar abundances (Venn+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/129">J/A+A/439/129 : HERES II. 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Uncertainty in logeps</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ei</name><description>[0.0/0.86]? Statistical abundance uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sX</name><description>[0.0/0.83]? Systematic abundance uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>delTeff</name><description>[-0.19/0.52]? Abundance difference from stellar effective temperature uncertainty</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dellogg</name><description>[-0.87/0.44]? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ion</name><description>Ion identifier</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Num</name><description>[1/130] Number of lines used</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_logeps</name><description>Formal 5{sigma} upper limit flag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logeps</name><description>[-2.22/9.02] log abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[X/H]</name><description>[-4.24/1.01] log abundance relative to H</description><ucd>phys.abund;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[X/H]</name><description>[0.04/0.63]? 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