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Activity indicators and stellar parameters of the Kepler targets An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra
Frasca, A.1; Molenda-Zakowicz, J.2,3; De Cat, P.4; Catanzaro, G.1; Fu, J. N.5; Ren, A. B.5; Luo, A. L.6; Shi, J. R.6; Wu, Y.6; Zhang, H. T.6
2016-10-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume594
AbstractAims. A comprehensive and homogeneous determination of stellar parameters for the stars observed by the Kepler space telescope is necessary for statistical studies of their properties. As a result of the large number of stars monitored by Kepler, the largest and more complete databases of stellar parameters published to date are multiband photometric surveys. The LAMOST-Kepler survey, whose spectra are analyzed in the present paper, was the first large spectroscopic project, which started in 2011 and aimed at filling that gap. In this work we present the results of our analysis, which is focused on selecting spectra with emission lines and chromospherically active stars by means of the spectral subtraction of inactive templates. The spectroscopic determination of the atmospheric parameters for a large number of stars is a by-product of our analysis.
SubtypeArticle
KeywordSurveys Techniques: Spectroscopic Stars: Fundamental Parameters Stars: Kinematics And Dynamics Stars: Activity Stars: Chromospheres
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationNational Development and Reform Commission ; National Development and Reform Commission ; Italian Ministero dell'Istruzione, Universite, e Ricerca (MIUR) ; Italian Ministero dell'Istruzione, Universite, e Ricerca (MIUR) ; European Community(269194 ; European Community(269194 ; Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC)(U1231202) ; Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC)(U1231202) ; Chinese Academy of Sciences(U1231202) ; Chinese Academy of Sciences(U1231202) ; National Basic Research Program of China (973 Program)(2014CB845700 ; National Basic Research Program of China (973 Program)(2014CB845700 ; National Science Foundation of China (NSFC)(11403056) ; National Science Foundation of China (NSFC)(11403056) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; NCN 2014/13/B/ST9/00902) ; NCN 2014/13/B/ST9/00902) ; 2013CB834900) ; 2013CB834900) ; National Development and Reform Commission ; National Development and Reform Commission ; Italian Ministero dell'Istruzione, Universite, e Ricerca (MIUR) ; Italian Ministero dell'Istruzione, Universite, e Ricerca (MIUR) ; European Community(269194 ; European Community(269194 ; Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC)(U1231202) ; Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC)(U1231202) ; Chinese Academy of Sciences(U1231202) ; Chinese Academy of Sciences(U1231202) ; National Basic Research Program of China (973 Program)(2014CB845700 ; National Basic Research Program of China (973 Program)(2014CB845700 ; National Science Foundation of China (NSFC)(11403056) ; National Science Foundation of China (NSFC)(11403056) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; NCN 2014/13/B/ST9/00902) ; NCN 2014/13/B/ST9/00902) ; 2013CB834900) ; 2013CB834900)
DOI10.1051/0004-6361/201628337
WOS KeywordDIGITAL SKY SURVEY ; LATE-TYPE STARS ; GENEVA-COPENHAGEN SURVEY ; MEAN RADIAL-VELOCITIES ; MAIN-SEQUENCE STARS ; 1ST DATA RELEASE ; FIELD-OF-VIEW ; A-TYPE STARS ; F-TYPE STARS ; ATMOSPHERIC PARAMETERS
Indexed BySCI
Language英语
Funding OrganizationNational Development and Reform Commission ; National Development and Reform Commission ; Italian Ministero dell'Istruzione, Universite, e Ricerca (MIUR) ; Italian Ministero dell'Istruzione, Universite, e Ricerca (MIUR) ; European Community(269194 ; European Community(269194 ; Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC)(U1231202) ; Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC)(U1231202) ; Chinese Academy of Sciences(U1231202) ; Chinese Academy of Sciences(U1231202) ; National Basic Research Program of China (973 Program)(2014CB845700 ; National Basic Research Program of China (973 Program)(2014CB845700 ; National Science Foundation of China (NSFC)(11403056) ; National Science Foundation of China (NSFC)(11403056) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; NCN 2014/13/B/ST9/00902) ; NCN 2014/13/B/ST9/00902) ; 2013CB834900) ; 2013CB834900) ; National Development and Reform Commission ; National Development and Reform Commission ; Italian Ministero dell'Istruzione, Universite, e Ricerca (MIUR) ; Italian Ministero dell'Istruzione, Universite, e Ricerca (MIUR) ; European Community(269194 ; European Community(269194 ; Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC)(U1231202) ; Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC)(U1231202) ; Chinese Academy of Sciences(U1231202) ; Chinese Academy of Sciences(U1231202) ; National Basic Research Program of China (973 Program)(2014CB845700 ; National Basic Research Program of China (973 Program)(2014CB845700 ; National Science Foundation of China (NSFC)(11403056) ; National Science Foundation of China (NSFC)(11403056) ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; NCN 2014/13/B/ST9/00902) ; NCN 2014/13/B/ST9/00902) ; 2013CB834900) ; 2013CB834900)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000385832200061
Citation statistics
Cited Times:23[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8280
Collection光学天文研究部
Affiliation1.INAF Osservatorio Astrofis Catania, Via S Sofia 78, I-95123 Catania, Italy
2.Univ Wroclaw, Astron Inst, Ul Kopernika 11, PL-51622 Wroclaw, Poland
3.New Mexico State Univ, Dept Astron, Las Cruces, NM 88003 USA
4.Royal Observ Belgium, Ringlaan 3, B-1180 Brussels, Belgium
5.Beijing Normal Univ, Dept Astron, 19 Ave Xinjiekouwai, Beijing 100875, Peoples R China
6.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Frasca, A.,Molenda-Zakowicz, J.,De Cat, P.,et al. Activity indicators and stellar parameters of the Kepler targets An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra[J]. ASTRONOMY & ASTROPHYSICS,2016,594.
APA Frasca, A..,Molenda-Zakowicz, J..,De Cat, P..,Catanzaro, G..,Fu, J. N..,...&Zhang, H. T..(2016).Activity indicators and stellar parameters of the Kepler targets An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.ASTRONOMY & ASTROPHYSICS,594.
MLA Frasca, A.,et al."Activity indicators and stellar parameters of the Kepler targets An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra".ASTRONOMY & ASTROPHYSICS 594(2016).
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