The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)

By X. Cui, Yongheng Zhao, Y. Chu, Guo-ping Li, Qi Li, Liping Zhang, H. Su, Zheng-qiu Yao, Ya-nan Wang, X. Xing and 67 more. 2012

660 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/abf67cecd52bb7dfc2f15161fbd79218895e3583

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Chao Liu
2. Jun-Chen Wan
3. Licai Deng
4. Petr Jelínek
5. Zhanwen Han
6. Yan-Chuan Cai
7. A. Luo
8. Xuelei Chen

In Atomic and Molecular Physics, and Optics

1. Yue Wu

In Instrumentation

1. Chao Liu
2. Jun-Chen Wan
3. Licai Deng
4. A. Luo
5. J. McLaughlin
6. Petr Jelínek
7. Jianling Wang
8. Valery M. Nakariakov

Citations in the corpus

• Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares (2018, methodology): “Karoff et al. (2016) analysed 48 superflare stars using the LAMOST telescope (Cui et al. 2012) and suggested that solar flares and superflares most likely share the same underlying mechanism.3 Furthermore, there has been a wealth of QPP detections in stellar flares using NASA’s Kepler mission…”
• The first data release (DR1) of the LAMOST regular survey (2015, methodology): “In general, the throughputs of the red and blue channels are 4% and 2% respectively (Cui et al. 2012).”
• THE VERTICAL METALLICITY GRADIENT OF THE MILKY WAY DISK: TRANSITIONS IN [α/Fe] POPULATIONS (2014, neutral): “We eagerly await upcoming data from GaiaESO (Gilmore et al. 2012), the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (Cui et al. 2012), GALAH (Zucker et al. 2012), and APOGEE (Ahn et al. 2014), which may be better able to constrain the disk chemical and dynamical structure.”
• PLATO as it is: a legacy mission for Galactic archaeology (2017, neutral): “…et al. 2011; Yanny et al. 2009), APOGEE (Majewski et al. 2015; Majewski, APOGEE Team, & APOGEE-2016), Gaia-ESO (Gilmore et al. 2012), LAM-OST (Cui et al. 2012), GALAH (De Silva et al. 2015; Martell et al. 2017), WEAVE (Dalton et al. 2014), 4MOST (de Jong et al. 2014), DESI (DESI…”
• Mapping the Milky Way with LAMOST– III. Complicated spatial structure in the outer disc (2018, methodology): “Therefore, we use the RGB stars observed in the LAMOST survey (Cui et al. 2012; MNRAS 000, 1–15 (2017) Zhao et al. 2012; Deng et al. 2012) to probe the structures of the outer disc.”