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<ri:Resource created="2000-04-12T21:40:48Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" 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/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>Spectroscopy of hot stars in the halo</title><shortName>J/AJ/117/2308</shortName><identifier>ivo://CDS.VizieR/J/AJ/117/2308</identifier><altIdentifier>doi:10.26093/cds/vizier.51172308</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wilhelm R.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Gray R.O.</name></creator><date role="Updated">2023-04-06T16:50:32Z</date><date role="Created">2000-04-12T21:40:48Z</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>metallicity</subject><subject>two-color-diagrams</subject><subject>line-intensities</subject><subject>astronomical-models</subject><subject>stellar-atmospheres</subject><subject>halo-stars</subject><subject>horizontal-branch-stars</subject><description>We discuss a spectroscopic and photometric technique that enables the identification and classification of field horizontal-branch (FHB) and other A-type stars, even from relatively low signal-to-noise ratio medium-resolution spectra. This technique makes use of broadband UBV colors predicted from model atmosphere calculations and Balmer line profiles and Ca II K equivalent widths determined from synthetic spectra to estimate the physical parameters T_eff_, log(g), and [Fe/H] for stars in the effective temperature range 6000 - 10,000 K.</description><source format="bibcode">1999AJ....117.2308W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/117/2308</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>related-to</relationshipType><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/VI/39">VI/39 : Model Atmospheres (Kurucz, 1979)</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/117/2308</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/117/2308</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/117/2308</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/117/2308</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/117/2308</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/117/2308</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/AJ/117/2308/table1</name><description>Calibration grid from Kurucz model atmospheres</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Temp</name><description>Effective temperature of Kurucz model</description><unit>K</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(g)</name><description>Log of the surface gravity of Kurucz model</description><unit>log(g.cm**-2)</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Log of the iron abundance relative to hydrogen of Kurucz model</description><unit>log(Sun)</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B-V</name><description>Predicted B-V from Kurucz color calibrations</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>U-B</name><description>Predicted U-B from Kurucz color calibrations</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EqWCa</name><description>Equivalent width of the Ca II K line</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EqWH4</name><description>Equivalent width of H{delta}</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EqWH3</name><description>Equivalent width of H{gamma}</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DH4</name><description>Full width at 20% below a local continuum level of H{delta}</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DH3</name><description>Full width at 20% below a local continuum level of H{gamma}</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>