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Related papers: A Large Sample of Am Candidates from LAMOST Data R…

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LAMOST DR5 released more than 200,000 low resolution spectra of early-type stars with S/N>50. Searching for metallic-line (Am) stars in such a large database and study of their statistical properties are presented in this paper. Six machine…

Solar and Stellar Astrophysics · Physics 2019-06-05 Li Qin , A-Li Luo , Wen Hou , Yin-Bi Li , Shuo Zhang , Rui Wang , Li-Li Wang , Xiao Kong , Jin-Shu Han

Since the release of LAMOST (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope) catalog, we have the opportunity to use the LAMOST DR2 stellar catalog and \emph{WISE All-sky catalog} to search for 22 $\mu$m excess candidates. In…

Solar and Stellar Astrophysics · Physics 2016-07-13 Chao-Jian Wu , Hong Wu , Kang Liu , Tan-Da Li , Ming Yang , Man I Lam , Fan Yang , Yue Wu , Yong Zhang , Yonghui Hou , Guangwei Li

Lithium is a fragile but crucial chemical element in the universe, exhibits interesting and complex behaviors. Thanks to the massive spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)…

Recently the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) published its first data release (DR1), which is ranked as the largest stellar spectra dataset in the world so far. We combine the PASTEL catalog and SIMBAD…

Solar and Stellar Astrophysics · Physics 2015-12-16 Hua Gao , Huawei Zhang , Maosheng Xiang , Yang Huang , Xiaowei Liu , Ali Luo , Haotong Zhang , Yue Wu , Yong Zhang , Guangwei Li , Bing Du

In this work, we present new catalogs of M giant and M dwarf stars from the LAMOST DR5. In total, 39,796 M giants and 501,152 M dwarfs are identified from the classification pipeline. The template-fitting results contain M giants with 7…

Astrophysics of Galaxies · Physics 2019-09-25 Jing Zhong , Jing Li , Jeffrey L. Carlin , Li Chen , Rene A. Mendez , Jinliang Hou

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Low Resolution Spectroscopic Survey (LRS) provides massive spectroscopic data of M-type stars, and the derived stellar parameters could bring vital help to various…

We present a catalog of 8,440 candidate very metal-poor (VMP; [Fe/H] < -2.0) main-sequence turn-off (MSTO) and red giant stars in the Milky Way, identified from low-resolution spectra in LAMOST DR10. More than 7,000 of these candidates are…

Astrophysics of Galaxies · Physics 2025-06-12 Xiangyu Li , Huiling Chen , Yang Huang , Huawei Zhang , Timothy C. Beers , Linxuan Zhu , Jifeng Liu

We present a value-added catalog containing stellar parameters estimated from 7.10 million low-resolution spectra for 5.16 million unique stars with spectral signal-to-noise ratios (SNRs) higher than 10 obtained by the Large Sky Area…

Solar and Stellar Astrophysics · Physics 2022-04-06 Chun Wang , Yang Huang , Haibo Yuan , Huawei Zhang , Maosheng Xiang , Xiaowei Liu

M dwarfs are the most common type of star in the Galaxy, and because of their small size are favored targets for searches of Earth-sized transiting exoplanets. Current and upcoming all-sky spectroscopic surveys, such as the Large Sky Area…

Solar and Stellar Astrophysics · Physics 2020-04-15 Brianna Galgano , Keivan Stassun , Barbara Rojas-Ayala

In this work, we present a catalog of 2651 carbon stars from the fourth Data Release (DR4) of the Large Sky Area Multi-Object Fiber Spectroscopy Telescope (LAMOST). Using an efficient machine-learning algorithm, we find out these stars from…

Low-mass emission-line stars belong to various evolutionary stages, from pre-main-sequence young stars to evolved stars. In this work, we present a catalog of late-type (F0 to M9) emission-line stars from the LAMOST Data Release 6. Using…

Solar and Stellar Astrophysics · Physics 2024-10-24 D. Edwin , Blesson Mathew , B. Shridharan , Vineeth Valsan , S. Nidhi , Suman Bhattacharyya , Sreeja S. Kartha , T. Robin

The abundance patterns of $r$-process-enhanced stars contain key information required to constrain the astrophysical site(s) of $r$-process nucleosynthesis, and to deepen our understanding of the chemical evolution of our Galaxy. In order…

Solar and Stellar Astrophysics · Physics 2021-03-31 Tian-Yi Chen , Jian-Rong Shi , Timothy C. Beers , Hong-Liang Yan , Qi Gao , Chun-Qian Li , Hai-Ning Li , Gang Zhao

Metal-poor (MP) stars are important targets for investigating the chemical evolution of the early universe. Among them, Carbon-Enhanced Metal-Poor (CEMP) stars have attracted extensive attention due to their rarity and astrophysical…

Solar and Stellar Astrophysics · Physics 2026-03-26 Xianqi Liu , Xiangru Li , Ziyu Fang

In this work, we provide 2189 photometric- and kinematic-selected member candidates of 24 star clusters from the LAMOST DR2 catalog. We perform two-step membership identification: selection along the stellar track in the color-magnitude…

Solar and Stellar Astrophysics · Physics 2016-01-26 Bo Zhang , Xiao-Yan Chen , Chao Liu , Li Chen , Li-Cai Deng , Jin-Liang Hou , Zheng-Yi Shao , Fan Yang , Yue Wu , Ming Yang , Yong Zhang , Yong-Hui Hou , Yue-Fei Wang

We derive stellar parameters and abundances (`stellar labels') of 40,034 late-B and A-type main-sequence stars extracted from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope Medium Resolution Survey (LAMOST--MRS). The primary…

Solar and Stellar Astrophysics · Physics 2021-11-17 Weijia Sun , Xiao-Wei Duan , Licai Deng , Richard de Grijs , Bo Zhang , Chao Liu

The LAMOST-Kepler/K2 Medium-Resolution Spectroscopic Survey (LK-MRS) conducted time-domain medium-resolution spectroscopic observations of 20 LAMOST plates in the Kepler and K2 fields from 2018 to 2023, a phase designated as LK-MRS-I. A…

We report on searching for Classical B-type emission-line (CBe) stars from the first data release (DR1) of the Large Sky Area Multi-Object fiber Spectroscopic Telescope (LAMOST; also named the Guoshoujing Telescope). A total of 192 (12…

Solar and Stellar Astrophysics · Physics 2015-05-28 C. C. Lin , J. L. Hou , L. Chen , Z. Y. Shao , J. Zhong , P. C. Yu

A sample of 70 E+A galaxies are selected from 37, 206 galaxies in the second data release (DR2) of Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) according to the criteria for E+A galaxies defined by Goto, and each of…

We report on early results from a pilot program searching for metal-poor stars with LAMOST and follow-up high-resolution observation acquired with the MIKE spectrograph attached to the Magellan~II telescope. We performed detailed abundance…

Solar and Stellar Astrophysics · Physics 2015-01-14 Hai-Ning Li , Gang Zhao , Norbert Christlieb , Liang Wang , Wei Wang , Yong Zhang , Yonghui Hou , Hailong Yuan

The Large sky Area Multi-Object Spectroscopic Telescope (LAMOST) General Survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs.…

Astrophysics of Galaxies · Physics 2020-07-22 A. -L. Luo , Y. -H. Zhao , G. Zhao , L. -C. Deng , X. -W. Liu , Y. -P. Jing , G. Wang , H. -T Zhang , J. -R. Shi , X. -Q. Cui , Y. -Q. Chu , G. -P. Li , Z. -R. Bai , Y. Cai , S. -Y. Cao , Z. -H Cao , J. L. Carlin , H. Y. Chen , J. -J. Chen , K. -X. Chen , L. Chen , X. -L. Chen , X. -Y. Chen , Y. Chen , N. Christlieb , J. -R. Chu , C. -Z. Cui , Y. -Q. Dong , B. Du , D. -W. Fan , L. Feng , J. -N Fu , P. Gao , X. -F. Gong , B. -Z. Gu , Y. -X. Guo , Z. -W. Han , B. -L. He , J. -L. Hou , Y. -H. Hou , W. Hou , H. -Z. Hu , N. -S. Hu , Z. -W. Hu , Z. -Y. Huo , L. Jia , F. -H. Jiang , X. Jiang , Z. -B. Jiang , G. Jin , X. Kong , X. Kong , Y. -J. Lei , A. -H. Li , C. -H. Li , G. -W. Li , H. -N. Li , J. Li , Q. Li , S. Li , S. -S. Li , X. -N. Li , Y. Li , Y. -B. Li , Y. -P. Li , Y. Liang , C. -C. Lin , C. Liu , G. -R. Liu , G. -Q. Liu , Z. -G. Liu , W. -Z. Lu , Y. Luo , Y. -D. Mao , H. Newberg , J. -J. Ni , Z. -X. Qi , Y. -J. Qi , S. -Y. Shen , H. -M. Shi , J. Song , Y. -H. Song , D. -Q. Su , H. -J. Su , Z. -H. Tang , Q. -S. Tao , Y. Tian , D. Wang , D. -Q. Wang , F. -F. Wang , G. -M. Wang , H. Wang , H. -C. Wang , J. Wang , J. -N. Wang , J. -L. Wang , J. -P. Wang , J. -X. Wang , L. Wang , M. -X. Wang , S. -G. Wang , S. -Q. Wang , X. Wang , Y. -N. Wang , Y. Wang , Y. -F. Wang , Y. -F. Wang , P. Wei , M. -Z. Wei , H. Wu , K. -F. Wu , X. -B. Wu , Y. Wu , Y. Z. Wu , X. -Z. Xing , L. -Z. Xu , X. -Q. Xu , Y. Xu , T. -S. Yan , D. -H. Yang , H. -F. Yang , H. -Q. Yang , M. Yang , Z. -Q. Yao , Y. Yu , H. Yuan , H. -B. Yuan , H. -L. Yuan , W. -M. Yuan , C. Zhai , E. -P. Zhang , H. W. Zhang , J. -N. Zhang , L. -P. Zhang , W. Zhang , Y. Zhang , Y. -X. Zhang , Z. -C. Zhang , M. Zhao , F. Zhou , X. Zhou , J. Zhu , Y. -T. Zhu , S. -C. Zou , F. Zuo
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