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	Magnetic Activity of F-, G-, and K-type Stars in the LAMOST-Kepler Field
	Zhang, Jinghua1; Bi, Shaolan1; Li, Yaguang1; Jiang, Jie2; Li, Tanda3,4; He, Han5; Yu, Jie6; Khanna, Shourya3; Ge, Zhishuai7; Liu, Kang1; Tian, Zhijia8; Wu, Yaqian9; Zhang, Xianfei1
	2020-03-01
Source Publication	ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
ISSN	0067-0049
Volume	247Issue:1Pages:8
Abstract	Monitoring chromospheric and photospheric indexes of magnetic activity can provide valuable information, especially the interaction between different parts of the atmosphere and their response to magnetic fields. We extract chromospheric indexes, S and R-HK(+), for 59,816 stars from LAMOST spectra in the LAMOST-Kepler program, and photospheric index, R-eff, for 5575 stars from Kepler light curves. The log Reff shows positive correlation with log R-HK(+). We estimate the power-law indexes between Reff and R-HK(+) for F-, G-, and K-type stars, respectively. We also confirm the dependence of both chromospheric and photospheric activity on stellar rotation. Ca II H and K emissions and photospheric variations generally decrease with increasing rotation periods for stars with rotation periods exceeding a few days. The power-law indexes in exponential decay regimes show different characteristics in the two activity-rotation relations. The updated largest sample including the activity proxies and reported rotation periods provides more information to understand the magnetic activity for cool stars.
Funding Organization	National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Youth Scholars Program of Beijing Normal University ; Australian Research Council ; Australian Research Council ; Danish National Research Foundation ; Danish National Research Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; Alibaba Cloud ; NASA's Science Mission Directorate ; NASA's Science Mission Directorate ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Youth Scholars Program of Beijing Normal University ; Australian Research Council ; Australian Research Council ; Danish National Research Foundation ; Danish National Research Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; Alibaba Cloud ; NASA's Science Mission Directorate ; NASA's Science Mission Directorate ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Youth Scholars Program of Beijing Normal University ; Australian Research Council ; Australian Research Council ; Danish National Research Foundation ; Danish National Research Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; Alibaba Cloud ; NASA's Science Mission Directorate ; NASA's Science Mission Directorate ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Youth Scholars Program of Beijing Normal University ; Australian Research Council ; Australian Research Council ; Danish National Research Foundation ; Danish National Research Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; Alibaba Cloud ; NASA's Science Mission Directorate ; NASA's Science Mission Directorate ; National Development and Reform Commission ; National Development and Reform Commission
DOI	10.3847/1538-4365/ab6165
WOS Keyword	SUN-LIKE STARS ; CA-II H ; COOL STARS ; CHROMOSPHERIC ACTIVITY ; LINEAR-REGRESSION ; RADIATIVE LOSSES ; STELLAR ACTIVITY ; SOLAR ; EMISSION ; ROTATION
Language	英语
Funding Project	National Natural Science Foundation of China (NSFC)[U1631236] ; Chinese Academy of Sciences (CAS)[U1631236] ; National Natural Science Foundation of China[11522325] ; National Natural Science Foundation of China[11873023] ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Australian Research Council[DP150104667] ; Danish National Research Foundation[DNRF106] ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; NASA's Science Mission Directorate ; National Development and Reform Commission
Funding Organization	National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Youth Scholars Program of Beijing Normal University ; Australian Research Council ; Australian Research Council ; Danish National Research Foundation ; Danish National Research Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; Alibaba Cloud ; NASA's Science Mission Directorate ; NASA's Science Mission Directorate ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Youth Scholars Program of Beijing Normal University ; Australian Research Council ; Australian Research Council ; Danish National Research Foundation ; Danish National Research Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; Alibaba Cloud ; NASA's Science Mission Directorate ; NASA's Science Mission Directorate ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Youth Scholars Program of Beijing Normal University ; Australian Research Council ; Australian Research Council ; Danish National Research Foundation ; Danish National Research Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; Alibaba Cloud ; NASA's Science Mission Directorate ; NASA's Science Mission Directorate ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Youth Scholars Program of Beijing Normal University ; Youth Scholars Program of Beijing Normal University ; Australian Research Council ; Australian Research Council ; Danish National Research Foundation ; Danish National Research Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; Alibaba Cloud ; NASA's Science Mission Directorate ; NASA's Science Mission Directorate ; National Development and Reform Commission ; National Development and Reform Commission
WOS Research Area	Astronomy & Astrophysics
WOS Subject	Astronomy & Astrophysics
WOS ID	WOS:000537501900002
Publisher	IOP PUBLISHING LTD
Citation statistics
Document Type	期刊论文
Identifier	http://ir.bao.ac.cn/handle/114a11/83490
Collection	中国科学院国家天文台
Corresponding Author	Bi, Shaolan
Affiliation	1.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China 2.Beihang Univ, Sch Space & Environm, Beijing 100083, Peoples R China 3.Univ Sydney, Sydney Inst Astron SIfA, Sch Phys, Sydney, NSW 2006, Australia 4.Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, Ny Munkegade 120, DK-8000 Aarhus C, Denmark 5.Chinese Acad Sci, Natl Astron Observ, CAS Key Lab Solar Act, Beijing 100101, Peoples R China 6.Max Planck Inst Solar Syst Res, D-37077 Gottingen, Germany 7.Minist Educ, Beijing Radiat Ctr, Key Lab Beam Technol, Beijing 100875, Peoples R China 8.Yunnan Univ, Sch Phys & Astron, Kunming 650091, Yunnan, Peoples R China 9.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100101, Peoples R China
Recommended Citation GB/T 7714	Zhang, Jinghua,Bi, Shaolan,Li, Yaguang,et al. Magnetic Activity of F-, G-, and K-type Stars in the LAMOST-Kepler Field[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2020,247(1):8.
APA	Zhang, Jinghua.,Bi, Shaolan.,Li, Yaguang.,Jiang, Jie.,Li, Tanda.,...&Zhang, Xianfei.(2020).Magnetic Activity of F-, G-, and K-type Stars in the LAMOST-Kepler Field.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,247(1),8.
MLA	Zhang, Jinghua,et al."Magnetic Activity of F-, G-, and K-type Stars in the LAMOST-Kepler Field".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 247.1(2020):8.

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