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<ri:Resource created="2020-09-09T16:03:36Z" 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>Catalog of FHB stars aligned with HVCs</title><shortName>J/ApJS/161/147</shortName><identifier>ivo://CDS.VizieR/J/ApJS/161/147</identifier><altIdentifier>doi:10.26093/cds/vizier.21610147</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Thom C.</name></creator><creator><name>Gibson B.K.</name></creator><creator><name>Christlieb N.</name></creator><date role="Updated">2020-11-30T07:48:28Z</date><date role="Created">2020-09-09T16:03:36Z</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>molecular-clouds</subject><subject>interstellar-medium</subject><description>We present a catalog of 430 field horizontal branch (FHB) stars, selected from the Hamburg/ESO Survey (HES), which fortuitously align with high column density neutral hydrogen (HI) high-velocity cloud (HVC) gas. These stars are ideal candidates for absorption-line studies of HVCs, attempts at which have been made for almost 40 years with little success. A parent sample of 8321 HES FHB stars (Christlieb et al., 2005, Cat. &lt;J/A+A/431/143&gt;) was used to extract HI spectra along each line of sight, using the HI Parkes All-Sky Survey (Putman et al., 2002, Cat. &lt;J/AJ/123/873&gt;). All lines of sight aligned with high-velocity HI emission with peak brightness temperatures greater than 120mK were examined. The HI spectra of these 430 probes were visually screened and cross-referenced with several HVC catalogs.</description><source format="bibcode">2005ApJS..161..147T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/161/147</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/A+A/431/143">J/A+A/431/143 : Field horizontal-branch stars in the Galaxy (Christlieb+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/873">J/AJ/123/873 : HIPASS high-velocity clouds (Putman+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/391/159">J/A+A/391/159 : A search for Compact High-Velocity Clouds (De Heij+, 2002)</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/161/147</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/161/147</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/161/147</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/161/147</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/161/147</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[TGC2005]</name><description>Running number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HEname</name><description>HES identification (Cat. &lt;J/A+A/431/143&gt;) (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>GLON</name><description>Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag</name><description>The HES B band magnitude (2)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>Distance (3)</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb</name><description>Peak brightness temperature (4)</description><unit>K</unit><ucd>phys.temperature;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NHI</name><description>HI column density along the line-of-sight</description><unit>cm**-2</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VLSR</name><description>LSR velocity of the peak HI emission (5)</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MS</name><description>[*] Association with the Magellanic Stream</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>HVCtyp</name><description>HVC type from Putman et al. (2002, Cat. &lt;J/AJ/123/873&gt;) (6)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>HVC</name><description>? Putman et al. (2002, Cat. &lt;J/AJ/123/873&gt;) HVC name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>XHVCtyp</name><description>XHVC type Putman et al. (2002, Cat. &lt;J/AJ/123/873&gt;) (6)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>XHVC</name><description>? Putman et al. (2002, Cat. &lt;J/AJ/123/873&gt;) XHVC name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>WvW91</name><description>? 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