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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
发表期刊ASTRONOMY & ASTROPHYSICS
卷号594
摘要Aims. 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.
文章类型Article
关键词Surveys Techniques: Spectroscopic Stars: Fundamental Parameters Stars: Kinematics And Dynamics Stars: Activity Stars: Chromospheres
WOS标题词Science & Technology ; Physical Sciences
资助者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) ; 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
关键词[WOS]DIGITAL 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
收录类别SCI
语种英语
资助者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) ; 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研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000385832200061
引用统计
被引频次:15[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8280
专题光学天文研究部
作者单位1.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
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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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