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<ri:Resource created="2005-12-01T11:58:30Z" 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>BHB stars in Century Survey Galactic Halo Project</title><shortName>J/AJ/130/1097</shortName><identifier>ivo://CDS.VizieR/J/AJ/130/1097</identifier><altIdentifier>doi:10.26093/cds/vizier.51301097</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brown W.R.</name></creator><creator><name>Geller M.J.</name></creator><creator><name>Kenyon S.J.</name></creator><creator><name>Kurtz M.J.</name></creator><creator><name>Allende Prieto C.,Beers T.C.</name></creator><creator><name>Wilhelm R.</name></creator><date role="Updated">2017-06-13T11:08:14Z</date><date role="Created">2005-12-01T11:58:30Z</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>horizontal-branch-stars</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>infrared-photometry</subject><description>We discuss a 175{deg}2 spectroscopic survey for blue horizontal branch (BHB) stars in the Galactic halo. We use the Two Micron All Sky Survey (2MASS, &lt;II/246&gt;) and the Sloan Digital Sky Survey (SDSS) to select BHB candidates, and we find that the 2MASS and SDSS color selection is 38% and 50% efficient, respectively, for BHB stars. Our samples include one likely runaway B7 star 6kpc below the Galactic plane.</description><source format="bibcode">2005AJ....130.1097B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/130/1097</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>http://www.sdss.org : The Sloan Digital Sky Survey home page</relatedResource><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/J/AJ/126/1362">J/AJ/126/1362 : Century Survey Galactic Halo Project. I. 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