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<ri:Resource created="2015-12-04T15:27:36Z" 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>Metal-poor stars from HES survey. II. Spectroscopy</title><shortName>J/ApJ/781/40</shortName><identifier>ivo://CDS.VizieR/J/ApJ/781/40</identifier><altIdentifier>doi:10.26093/cds/vizier.17810040</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Placco V.M.</name></creator><creator><name>Frebel A.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Christlieb N.</name></creator><creator><name>Lee Y.S.</name></creator><creator><name>Kennedy C.R.,Rossi S.</name></creator><creator><name>Santucci R.M.</name></creator><date role="Updated">2017-12-06T07:38:31Z</date><date role="Created">2015-12-04T15:27:36Z</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>halo-stars</subject><subject>chemically-peculiar-stars</subject><subject>chemical-abundances</subject><subject>line-intensities</subject><description>We report on the discovery of seven low-metallicity stars selected from the Hamburg/ESO Survey, six of which are extremely metal-poor (EMP, [Fe/H]{&lt;=}-3.0), with four having [Fe/H]{&lt;=}-3.5. Chemical abundances or upper limits are derived for these stars based on high-resolution (R~35000) Magellan/MIKE spectroscopy, and are in general agreement with those of other very and extremely metal-poor stars reported in the literature. Accurate metallicities and abundance patterns for stars in this metallicity range are of particular importance for studies of the shape of the metallicity distribution function of the Milky Way's halo system, in particular for probing the nature of its low-metallicity tail. In addition, taking into account suggested evolutionary mixing effects, we find that six of the program stars (with [Fe/H]{&lt;=}-3.35) possess atmospheres that were likely originally enriched in carbon, relative to iron, during their main-sequence phases. These stars do not exhibit overabundances of their s-process elements, and hence may be, within the error bars, additional examples of the so-called CEMP-no class of objects.</description><source format="bibcode">2014ApJ...781...40P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/781/40</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/J/ApJ/778/56">J/ApJ/778/56 : Hamburg/ESO Survey extremely metal-poor stars (Cohen+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/769/57">J/ApJ/769/57 : Equivalent widths of metal-poor stars (Frebel+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/762/26">J/ApJ/762/26 : Most metal-poor stars. II. Galactic halo stars (Yong+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/762/25">J/ApJ/762/25 : The most metal-poor stars in HES and SDSS. I. (Norris+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/188">J/AJ/142/188 : Metal-poor stars from the HES using CH G-band (Placco+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/1051">J/AJ/139/1051 : Carbon-enhanced metal-poor stars in the Galaxy (Placco+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/484/721">J/A+A/484/721 : HES survey. IV. Candidate metal-poor stars (Christlieb+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/652/1585">J/ApJ/652/1585 : Bright metal-poor stars from HES survey (Frebel+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/129">J/A+A/439/129 : HERES II. Spectroscopic analysis (Barklem+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/375/366">J/A+A/375/366 : Carbon stars from the Hamburg/ESO survey (Christlieb+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/103/1987">J/AJ/103/1987 : Stars of very low metal abundance (Beers+ 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/90/2089">J/AJ/90/2089 : Stars of very low metal abundance. I (Beers+, 1985)</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/781/40</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/781/40</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/781/40</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/781/40</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/781/40</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/781/40</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/781/40/table3 (Derived stellar parameters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/781/40/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/781/40/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/781/40/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>12.68875</ra><dec>-63.8638889</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/17095 33464 35695 45406 46311 46796 46813</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/781/40?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/781/40/table4</name><description>Abundances for individual species</description><column><name>Ion</name><description>Ion designation</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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