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<ri:Resource created="2016-06-22T08:21:21Z" 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>Parameters of Kepler stars using LAMOST &amp; seismic data</title><shortName>J/AJ/152/6</shortName><identifier>ivo://CDS.VizieR/J/AJ/152/6</identifier><altIdentifier>doi:10.26093/cds/vizier.51520006</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang L.</name></creator><creator><name>Wang W.</name></creator><creator><name>Wu Y.</name></creator><creator><name>Zhao G.</name></creator><creator><name>Li Y.</name></creator><creator><name>Luo A.</name></creator><creator><name>Liu C.</name></creator><creator><name>Zhang Y.</name></creator><creator><name>Hou Y.,Wang Y.</name></creator><creator><name>Cao Z.</name></creator><date role="Updated">2019-10-10T12:56:05Z</date><date role="Created">2016-06-22T08:21:21Z</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>effective-temperature</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>spectroscopy</subject><subject>metallicity</subject><description>Asteroseismology is a powerful tool to precisely determine the evolutionary status and fundamental properties of stars. With the unprecedented precision and nearly continuous photometric data acquired by the NASA Kepler mission, parameters of more than 10^4^ stars have been determined nearly consistently. However, most studies still use photometric effective temperatures (Teff) and metallicities ([Fe/H]) as inputs, which are not sufficiently accurate as suggested by previous studies. We adopted the spectroscopic Teff and [Fe/H] values based on the LAMOST low-resolution spectra (R~1,800), and combined them with the global oscillation parameters to derive the physical parameters of a large sample of stars. Clear trends were found between {Delta}logg(LAMOST-seismic) and spectroscopic Teff as well as logg, which may result in an overestimation of up to 0.5dex for the logg of giants in the LAMOST catalog. We established empirical calibration relations for the logg values of dwarfs and giants. These results can be used for determining the precise distances to these stars based on their spectroscopic parameters.</description><source format="bibcode">2016AJ....152....6W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/152/6</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/V/146">V/146 : LAMOST DR1 catalogs (Luo+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/525/A131">J/A+A/525/A131 : Kepler red giants Solar-like oscillations (Hekker+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/112">J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/540/A143">J/A+A/540/A143 : Red giants oscillations observed by Kepler (Mosser+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/543/A160">J/A+A/543/A160 : 82 Kepler red giants normalized spectra (Thygesen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/423/122">J/MNRAS/423/122 : Abundances of 93 solar-type Kepler targets (Bruntt+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/749/152">J/ApJ/749/152 : 22 solar-type stars asteroseismic analysis (Mathur+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/30">J/ApJS/199/30 : KIC stars effective temperature scale (Pinsonneault+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/486.375">J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/127">J/ApJ/767/127 : Asteroseismic solutions for 77 Kepler stars (Huber+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/L41">J/ApJ/765/L41 : Asteroseismic classification of KIC objects (Stello+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/434/1422">J/MNRAS/434/1422 : 169 FGKM stars atmospheric param. (Molenda-Zakowicz+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/1">J/ApJS/210/1 : Asteroseismic study of solar-type stars (Chaplin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/210/20">J/ApJS/210/20 : Small Kepler planets radial velocities (Marcy+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/2">J/ApJS/211/2 : Q1-16 Kepler targets revised stellar prop. (Huber+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/19">J/ApJS/215/19 : APOKASC catalog of Kepler red giants (Pinsonneault+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/220/19">J/ApJS/220/19 : LAMOST obs. in the Kepler field. I. 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