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<ri:Resource created="2022-11-28T09:01:10Z" 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>Sp. follow-up of low-metallicity S-PLUS stars</title><shortName>J/ApJS/262/8</shortName><identifier>ivo://CDS.VizieR/J/ApJS/262/8</identifier><altIdentifier>doi:10.26093/cds/vizier.22620008</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Placco V.M.</name></creator><creator><name>Almeida-Fernandes F.</name></creator><creator><name>Arentsen A.</name></creator><creator><name>Lee Y.S.</name></creator><creator><name>Schoenell W.,Ribeiro T.</name></creator><creator><name>Kanaan A.</name></creator><date role="Updated">2024-02-06T12:47:47Z</date><date role="Created">2022-11-28T09:01:10Z</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>chemically-peculiar-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>chemical-abundances</subject><description>This work presents the medium-resolution (R~1500) spectroscopic follow-up of 522 low-metallicity star candidates from the Southern Photometric Local Universe Survey (S-PLUS). The objects were selected from narrowband photometry, taking advantage of the metallicity-sensitive S-PLUS colors. The follow-up observations were conducted with the Blanco and Gemini South telescopes, using the COSMOS and GMOS spectrographs, respectively. The stellar atmospheric parameters (Teff, logg, and [Fe/H]), as well as carbon and {alpha}-element abundances, were calculated for the program stars in order to assess the efficacy of the color selection. Results show that 92_-3_^+2^% of the observed stars have [Fe/H]&lt;=-1.0, 83_-3_^+3^% have [Fe/H]&lt;=-2.0, and 15_-3_^+3^% have [Fe/H]&lt;=-3.0, including two ultra metal-poor stars ([Fe/H]&lt;=-4.0). The 80th percentile for the metallicity cumulative distribution function of the observed sample is [Fe/H]=-2.04. The sample also includes 68 carbon-enhanced metal-poor stars. Based on the calculated metallicities, further S-PLUS color cuts are proposed, which can increase the fractions of stars with [Fe/H]&lt;=-1.0 and &lt;=-2.0 to 98% and 88%, respectively. Such high success rates enable targeted high-resolution spectroscopic follow-up efforts, as well as provide selection criteria for fiber-fed multiplex spectroscopic surveys.</description><source format="bibcode">2022ApJS..262....8P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/262/8</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/358">II/358 : SkyMapper Southern Sky Survey. 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(Norris+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/58">J/ApJ/794/58 : Metal-poor stars in the Galaxy thick disk (Beers+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/571/A47">J/A+A/571/A47 : Extensive linelist of CH in stellar atm. (Masseron+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/797/21">J/ApJ/797/21 : Carbon-enhanced metal-poor stars (Placco+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/579/A28">J/A+A/579/A28 : Abundances of 3 CEMP stars (Bonifacio+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/833/20">J/ApJ/833/20 : Carbon-enhanced metal-poor star abundances (Yoon+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/81">J/ApJ/835/81 : Bright metal-poor stars from HES Survey. II. (Beers+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/472/2963">J/MNRAS/472/2963 : Metallicities of Pristine stars (Youakim+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/256">J/AJ/155/256 : Sp. validation of RAVE metal-poor stars (Placco+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/870/122">J/ApJ/870/122 : Sp. of low-metallicity star candidates (Placco+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/891/39">J/ApJ/891/39 : LAMOST DR3 very metal-poor stars of the halo (Yuan+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/254/31">J/ApJS/254/31 : Phot. metallicities of stars in SkyMapper DR2 (Chiti+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/907/10">J/ApJ/907/10 : The VMP HK/HES stars (Limberg+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/913/11">J/ApJ/913/11 : Sp. follow-up of bright metal-poor stars (Limberg+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/259/60">J/ApJS/259/60 : SEGUE-2 updated stellar parameter pipeline (Rockosi+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/926/26">J/ApJ/926/26 : DTGs of metal-poor stars. 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