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<ri:Resource created="2021-08-06T13:04:24Z" 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>Hot subdwarf stars from Gaia DR2 &amp; LAMOST DR6+7. I.</title><shortName>J/ApJ/889/117</shortName><identifier>ivo://CDS.VizieR/J/ApJ/889/117</identifier><altIdentifier>doi:10.26093/cds/vizier.18890117</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lei Z.</name></creator><creator><name>Zhao J.</name></creator><creator><name>Nemeth P.</name></creator><creator><name>Zhao G.</name></creator><date role="Updated">2022-07-08T07:06:09Z</date><date role="Created">2021-08-06T13:04:24Z</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>subdwarf-stars</subject><subject>chemical-abundances</subject><subject>stellar-spectral-types</subject><description>182 single-lined hot subdwarf stars are identified by using spectra from the sixth and seventh data releases (DR6 and DR7) of the Large Sky Area Multi-Object Fibre Spectroscopic Telescope survey. We classified all the hot subdwarf stars using a canonical classification scheme, and got 89 sdB, 37 sdOB, 26 sdO, 24 He-sdOB, 3 He-sdO, and 3 He-sdB stars, respectively. Among these stars, 108 hot subdwarfs are newly discovered, while 74 stars were reported by previous catalogs. The atmospheric parameters of these stars were obtained by fitting the hydrogen (H) and helium (He) lines with non-local thermodynamic equilibrium model atmospheres. The atmospheric parameters confirm the two He sequences and the two subgroups of He-sdOB stars in our samples, which were found by previous studies in the T_eff_-log(nHe/nH) diagram. Our results demonstrate different origins of field hot subdwarf stars and extreme horizontal branch stars in globular clusters, and provide strict observational limits on the formation and evolution models of the different sub-types of these evolved objects. Based on the results, we evaluated the completeness of the Geier+ (2017, J/A+A/600/A50) catalog. We found the fraction of hot subwarf stars is between 10% and 60%, depending on the brightness of the sample. A more accurate estimation for the hot subdwarf fraction can be obtained when similar results from composite spectra will become available.</description><source format="bibcode">2020ApJ...889..117L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/889/117</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/III/137">III/137 : Spectroscopically Identified Hot Subdwarf Stars (Kilkenny+ 1988)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/65">VI/65 : Evolutionary models of evolved stars (Dorman+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/258">III/258 : Revised and updated First Byurakan Survey (FBS) (Mickaelian, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/164">V/164 : LAMOST DR5 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/419/596">J/ApJ/419/596 : Pop I UV radiation models (Dorman+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/287/867">J/MNRAS/287/867 : Edinburgh-Cape Blue Object Survey. 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(Moehler+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/446/4078">J/MNRAS/446/4078 : New white dwarf stars in SDSS DR10 (Kepler+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/576/A44">J/A+A/576/A44 : Hot subdwarf binaries from MUCHFUSS (Kupfer+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/818/202">J/ApJ/818/202 : Hot subdwarf stars in LAMOST DR1 (Luo+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/455/3413">J/MNRAS/455/3413 : New WD and subdwarf stars in SDSS DR12 (Kepler+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/600/A50">J/A+A/600/A50 : Catalog of hot subdwarf stars (Geier+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/618/A15">J/A+A/618/A15 : Parameters of EHB stars in {omega} Cen (Latour+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/868/70">J/ApJ/868/70 : Hot subdwarf stars from Gaia DR2 and LAMOST DR5 (Lei+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/621/A38">J/A+A/621/A38 : Gaia catalogue of hot subluminous stars (Geier+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/881/135">J/ApJ/881/135 : Hot subdwarf stars from Gaia2 &amp; LAMOST DR5. 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