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<ri:Resource created="2005-12-16T16:04:39Z" 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>UBV photometry of HK survey stars</title><shortName>J/ApJS/76/1001</shortName><identifier>ivo://CDS.VizieR/J/ApJS/76/1001</identifier><altIdentifier>doi:10.26093/cds/vizier.20761001</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Preston G.W.</name></creator><creator><name>Shectman S.A.</name></creator><creator><name>Beers T.C.</name></creator><date role="Updated">2017-07-12T06:59:50Z</date><date role="Created">2005-12-16T16:04:39Z</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>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>chemically-peculiar-stars</subject><subject>halo-stars</subject><description>Photoelectric UBV observations of 1782 stars are used to explore properties of the HK objective-prism survey conducted by Beers, Preston, and Shectman with the Curtis-Schmidt telescope of the Cerro Tololo Inter-American Observatory. We construct an intrinsic (U-B)0 versus (B-V)0 relation for blue horizontal branch stars and use it to derive estimates of E(B-V) color excesses in 50 survey fields. Comparison of these with the reddening maps of Burstein and Heiles indicates good agreement except in low-latitude fields toward the Galactic bulge. We describe qualitative features of the stellar content of the HK survey by use of unreddened two-color diagrams and indicate how the photometric data may prove useful in several applications. Finally, we use a halo density model to estimate the variation of completeness with apparent magnitude, B, in our catalog of field horizontal branch star candidates.</description><source format="bibcode">1991ApJS...76.1001P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/76/1001</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/AJ/90/2089">J/AJ/90/2089 : Stars of very low metal abundance. (Beers+, 1985)</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/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/ApJS/76/1001</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/76/1001</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/76/1001</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/76/1001</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/76/1001</mirrorURL><mirrorURL 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