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<ri:Resource created="2019-11-20T14:45:20Z" 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 and LAMOST DR5</title><shortName>J/ApJ/868/70</shortName><identifier>ivo://CDS.VizieR/J/ApJ/868/70</identifier><altIdentifier>doi:10.26093/cds/vizier.18680070</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">2020-03-26T14:17:07Z</date><date role="Created">2019-11-20T14:45:20Z</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>astronomical-object-identification</subject><subject>chemical-abundances</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>narrow-band-photometry</subject><subject>stellar-spectral-types</subject><description>We selected 4593 hot subdwarf candidates from the Gaia DR2 Hertzsprung-Russell (HR) diagram. By combining the sample with Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) DR5, we identified 294 hot subdwarf stars, including 169 sdB, 63 sdOB, 31 He-sdOB, 22 sdO, 7 He-sdO, and 2 He-sdB stars. The atmospheric parameters (e.g., Teff, logg, log(nHe/nH)) are obtained by fitting the hydrogen (H) and helium (He) line profiles with synthetic spectra. Two distinct He sequences of hot subdwarf stars are clearly presented in the Teff-logg diagram. We found that the He-rich sequence consists of the bulk of sdB and sdOB stars, as well as all of the He-sdB, He-sdO, and He-sdOB stars in our samples, while all the stars in the He-weak sequence belong to the sdO spectral type, combined with a few sdB and sdOB stars. We demonstrated that the combination of Gaia DR2 and LAMOST DR5 allows one to uncover a huge number of new hot subdwarf stars in our Galaxy.</description><source format="bibcode">2018ApJ...868...70L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/868/70</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/II/207">II/207 : Palomar-Green catalog UV-excess stellar objects (Green+ 1986)</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/153">V/153 : LAMOST DR4 catalogs (Luo+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/400/939">J/A+A/400/939 : Stellar parameters of 115 HQS sdB stars (Edelmann+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/380/1098">J/MNRAS/380/1098 : UV-upturn of elliptical galaxies model (Han+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A28">J/A+A/530/A28 : Priority targets for the MUCHFUSS project (Geier+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/427/2180">J/MNRAS/427/2180 : GALEX survey subdwarf atmospheric parameters (Nemeth+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/25">J/ApJ/764/25 : FUSE spectra analysis of hot subdwarf stars (Jenkins, 2013)</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/other/RAA/16.G7">J/other/RAA/16.G7 : Nearby M subdwarfs from LAMOST DR2 (Bai+, 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/616/A10">J/A+A/616/A10 : Open clusters GaiaDR2 HR diagrams (Gaia Collaboration, 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/ApJS/240/31">J/ApJS/240/31 : M-subdwarf research. 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