LAMOST Observations in the Kepler Field. II. Database of the Low-resolution Spectra from the Five-year Regular Survey
LAMOST Observations in the Kepler Field. II. Database of the Low-resolution Spectra from the Five-year Regular Survey
复制标题
开普勒场中的 LAMOST 观测。
DOI：
10.3847/1538-4365/aadf81
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发表时间：
2018-10
期刊：
影响因子：
--
通讯作者：
LAMOST
中科院分区：
文献类型：
--
作者：
Zong Weikai;Fu Jian-Ning;De Cat Peter;Shi Jianrong;Luo Ali;Zhang Haotong;Frasca A.;Corbally C. J.;Molenda-akowicz J.;Catanzaro G.;Gray R. O.;Wang Jiangtao;Pan Yang;Ren Anbing;Zhang Ruyuan;Jin Mengqi;Wu Yue;Dong Subo;Xie Ji-Wei;Zhang Wei;Hou Yonghui;LAMOST
LAMOST - 开普勒（LK -）项目旨在利用大天区面积多目标光纤光谱望远镜（LAMOST）对开普勒任务视场中的目标进行光谱后续观测。开普勒视场被划分为1（句子似乎不完整）
The LAMOST-Kepler (LK-) project was initiated to use the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) to make spectroscopic follow-up observations for the targets in the field of the Kepler mission. The Kepler field is divided into 14 subfields that are adapted to the LAMOST circular field with a diameter of 5°. During the regular survey phase of LAMOST, the LK-project took data from 2012 June to 2017 June and covered all 14 subfields at least twice. In particular, we describe in this paper the second Data Release of the LK-project, including all spectra acquired through 2015 May–2017 June together with the first round observations of the LK-project from 2012 June to 2014 September. The LK-project now counts 227,870 spectra of 156,390 stars, among which we have derived atmospheric parameters ( , Teff, and [Fe/H]) and heliocentric radial velocity for 173,971 spectra of 126,172 stars. These parameters were obtained with the most recent version of the LAMOST Stellar Parameter Pipeline v 2.9.7. Nearly one half, namely 76,283 targets, are observed both by the LAMOST and Kepler telescopes. These spectra, establishing a large spectroscopy library, will be useful for the entire astronomical community, particularly for planetary science and stellar variability on Kepler targets.
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DOI：
10.1111/j.1365-2966.2010.17978.x
发表时间：
2010-11
影响因子：
4.8
作者：
J. Molenda–Żakowicz;D. Latham;G. Catanzaro;A. Frasca;S. Quinn
通讯作者：
J. Molenda–Żakowicz;D. Latham;G. Catanzaro;A. Frasca;S. Quinn
关于开普勒星的金属性
影响因子：
7.9
作者：
Yang, X. H.;Zhang, Haotong;Jin, Ge;Zhang, Yong
通讯作者：
Zhang, Yong
LAMOST望远镜揭示，热木星的海王星表亲大多是富含重元素的恒星的单一后代
DOI：
10.1073/pnas.1711406115
发表时间：
2017-06
影响因子：
11.1
作者：
Dong Subo;Xie Ji-Wei;Zhou Ji-Lin;Zheng Zheng;Luo Ali
通讯作者：
Luo Ali
DOI：
10.1088/0004-637x/798/2/110
发表时间：
2015-01
期刊：
The Astrophysical Journal
影响因子：
--
作者：
Haining Li;Gang Zhao;N. Christlieb;Liang-Yao Wang;Wei Wang;Yong Zhang;Yong-Hui Hou;Hailong Yuan-Hailong
通讯作者：
Haining Li;Gang Zhao;N. Christlieb;Liang-Yao Wang;Wei Wang;Yong Zhang;Yong-Hui Hou;Hailong Yuan-Hailong
影响因子：
4.8
作者：
Z. F. Bostancı;T. Ak;T. Yontan;S. Bilir;T. Guver;S. Ak;O. Cakirli;O. Ozdarcan;E. Paunzen
通讯作者：
Z. F. Bostancı;T. Ak;T. Yontan;S. Bilir;T. Guver;S. Ak;O. Cakirli;O. Ozdarcan;E. Paunzen