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<ri:Resource created="2005-12-16T14:03:59Z" 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>Stars of very low metal abundance. I</title><shortName>J/AJ/90/2089</shortName><identifier>ivo://CDS.VizieR/J/AJ/90/2089</identifier><altIdentifier>doi:10.26093/cds/vizier.50902089</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Beers T.C.</name></creator><creator><name>Preston G.W.</name></creator><creator><name>Shectman S.A.</name></creator><date role="Updated">2021-09-17T08:22:14Z</date><date role="Created">2005-12-16T14:03:59Z</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>halo-stars</subject><subject>spectroscopy</subject><description>An objective-prism and a narrowband interference filter have been used in combination on the Curtis Schmidt telescope at CTIO to conduct a search for extremely metal-poor stars. The filter restricts the bandpass to the region around the H and K lines of CaII; the metal-poor candidates are those stars with weak or absent H and K. Slit spectra (1 A resolution) of some 450 candidates are used to measure equivalent widths of the CaII K line and Balmer features. A calibration of the K-line strength for giants in the metal-poor globular cluster NGC 6397 and field dwarfs and giants of known metallicity is used to identify survey candidates with metal abundance [Fe/H]&lt;=-2.0; a list of 134 such stars is presented. UBV photometry is used to distinguish between two groups of metal-poor stars: a group with objects near the main-sequence turnoff, on the subgiant branch, and on the giant branch; and a second group with objects on the red horizontal branch (RHB) and asymptotic giant branch (AGB). The RHB-AGB stars exhibit the well-known weak G-band effect; three CH-strong objects are identified among the subgiants.</description><source format="bibcode">1985AJ.....90.2089B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/90/2089</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/AJ/87/1515">J/AJ/87/1515 : UBV photometry of AB stars in halo (Pier, 1982)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/53/791">J/ApJS/53/791 : Spectroscopy of AB stars in halo (Pier, 1983)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/102/1392">J/PASP/102/1392 : UBV photometry from HK survey. (Doinidis+ 1990)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/103/973">J/PASP/103/973 : Photoelectric UBV from HK survey. (Doidinis+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/76/1001">J/ApJS/76/1001 : UBV photometry of HK survey stars (Preston+, 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/103/267">J/AJ/103/267 : Spectrocopy of hot stars in galactic halo (Beers+ 1992)</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/108/268">J/AJ/108/268 : HK survey emission-line candidates positions (Beers+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/108/538">J/AJ/108/538 : Metal-poor MS stars UBV photometry (Preston+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/1188">J/AJ/112/1188 : HK survey emission-line candidates (Beers+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/117/2329">J/AJ/117/2329 : Spectroscopy of hot stars in the halo. (Wilhelm+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/123/639">J/ApJS/123/639 : UBV photometry of metal-weak candidates (Norris+, 1999)</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/AJ/90/2089</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/90/2089</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/90/2089</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/90/2089</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/90/2089</mirrorURL><mirrorURL title="VizieR at 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