LAMOST OBSERVATIONS IN THE KEPLER FIELD. ANALYSIS OF THE STELLAR PARAMETERS MEASURED WITH LASP BASED ON LOW-RESOLUTION SPECTRA

	LAMOST OBSERVATIONS IN THE KEPLER FIELD. ANALYSIS OF THE STELLAR PARAMETERS MEASURED WITH LASP BASED ON LOW-RESOLUTION SPECTRA
	Ren, Anbing 1; Fu, Jianning 1; De Cat, Peter 2; Wu, Yue3 ; Yang, Xiaohu 1; Shi, Jianrong3 ; Luo, Ali3 ; Zhang, Haotong3 ; Dong, Subo 4; Zhang, Ruyuan 1
刊名	ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
	2016-08-01
卷号	225 期号:2
关键词	astronomical databases: miscellaneous stars: fundamental parameters stars: general stars: statistics
英文摘要	All 14 subfields of the Kepler field were observed at least once with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST, Xinglong Observatory, China) during the 2012-2014 observation seasons. There are 88,628 reduced spectra with a signal-to-noise ratio in the g band (S/N-g) >= 6 after the first round (2012-2014) of observations of the LAMOST-Kepler project (LK-project). By adopting the upgraded version of the LAMOST Stellar Parameter pipeline (LASP), we have determined the atmospheric parameters (T-eff, log g, and [Fe/H]) and heliocentric radial velocity v(rad) for 51,406 stars with 61,226 spectra. Compared with the atmospheric parameters derived from both high-resolution spectroscopy and asteroseismology for common stars in Huber et al., an external calibration of LASP atmospheric parameters was made, leading to the determination of the external errors for giants and dwarfs. Multiple spectroscopic observations of the same objects in the LK-project were used to estimate the internal uncertainties of the atmospheric parameters as a function of S/N-g with the unbiased estimation method. The LASP atmospheric parameters were calibrated based on both the external and internal uncertainties for the giants and dwarfs. A general statistical analysis of the stellar parameters leads to the discovery of 106 candidate metal-poor stars, 9 candidate very metal-poor stars, and 18 candidate high-velocity stars. Fitting formulae were obtained segmentally for both the calibrated atmospheric parameters of the LK-project and the Kepler Input Catalog (KIC) parameters with common stars. The calibrated atmospheric parameters and radial velocities of the LK-project will be useful for studying stars in the Kepler field.
WOS标题词	Science & Technology ; Physical Sciences
类目[WOS]	Astronomy & Astrophysics
研究领域[WOS]	Astronomy & Astrophysics
关键词[WOS]	METAL-POOR STARS ; SPECTROSCOPIC TELESCOPE LAMOST ; SOLAR-TYPE STARS ; F-TYPE STARS ; ATMOSPHERIC PARAMETERS ; DATA RELEASE ; GIANT STARS ; SKY SURVEY ; TARGETS ; ASTEROSEISMOLOGY
收录类别	SCI
语种	英语
WOS记录号	WOS:000382309500011
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/6884]
专题	国家天文台_光学天文研究部
作者单位	1.Beijing Normal Univ, Dept Astron, 19 Xinjiekouwai St, Beijing 100875, Peoples R China 2.Royal Observ Belgium, Ringlaan 3, B-1180 Brussels, Belgium 3.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China 4.Peking Univ, Kavli Inst Astron & Astrophys, Yi He Yuan Rd 5, Beijing 100871, Peoples R China 5.Chinese Acad Sci, Natl Astron Observ, Nanjing Inst Astron Opt & Technol, Nanjing 210042, Peoples R China
推荐引用方式 GB/T 7714	Ren, Anbing,Fu, Jianning,De Cat, Peter,et al. LAMOST OBSERVATIONS IN THE KEPLER FIELD. ANALYSIS OF THE STELLAR PARAMETERS MEASURED WITH LASP BASED ON LOW-RESOLUTION SPECTRA[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2016,225(2).
APA	Ren, Anbing.,Fu, Jianning.,De Cat, Peter.,Wu, Yue.,Yang, Xiaohu.,...&Du, Bing.(2016).LAMOST OBSERVATIONS IN THE KEPLER FIELD. ANALYSIS OF THE STELLAR PARAMETERS MEASURED WITH LASP BASED ON LOW-RESOLUTION SPECTRA.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,225(2).
MLA	Ren, Anbing,et al."LAMOST OBSERVATIONS IN THE KEPLER FIELD. ANALYSIS OF THE STELLAR PARAMETERS MEASURED WITH LASP BASED ON LOW-RESOLUTION SPECTRA".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 225.2(2016).