LAMOST spectral survey — An overview

By Gang Zhao, Yongheng Zhao, Y. Chu, Yipeng Jing, Licai Deng. 2012

788 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/6dd33c0f7d83c6cbc8e2ee544cee259518d6f474

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. Timothy C. Beers
2. Chao Liu
3. Brian Yanny
4. Hans-Walter Rix
5. Licai Deng
6. Jun-Chen Wan
7. Jo Bovy
8. N. Christlieb

In Instrumentation

1. Chao Liu
2. Timothy C. Beers
3. Licai Deng
4. Jun-Chen Wan
5. Brian Yanny
6. N. Christlieb
7. J. Sellwood
8. K. Pan

Citations in the corpus

• The first data release (DR1) of the LAMOST regular survey (2015, methodology): “In the pilot survey, both Galactic and extragal ctic surveys were conducted – these were named LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) and LAMOST ExtraGAlactic Survey (LEGAS), respectively (Zhao et al. 2012; Liu et al. 2015).”
• Metallicity distributions of mono-age stellar populations of the Galactic disc from the LAMOST Galactic spectroscopic surveys (2018, neutral): “Recently, robust ages for a million main-sequence turn-off and sub-giant stars (MSTO-SG), selected from the LAMOST Galactic spectroscopic surveys (Cui et al. 2012; Zhao et al. 2012; Deng et al. 2012; Liu et al. 2014; Yuan et al. 2015), have become available (Xiang et al. 2017a).”
• LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) — The survey's science plan (2012, background): “…four year Galactic structure survey plan presented here includes spectra for 2.5 million stars brighter thanr < 19 and an additional 5 million stars brighter thanr < 17; the actual distribution of magnitudes observed will depend on the throughput of the GSJT system (Zhao et al. 2012, this volume).”
• Red Clump Stars from LAMOST II: the outer disc of the Milky Way (2017, methodology): “In this work, we select RC stars obtained from the LAMOST survey (Cui et al. 2012; Zhao et al. 2012) as tracers and compare the structural parameters between younger and older RC populations.”
• Data release of the LAMOST pilot survey (2012, methodology): “This effort will provide useful data for the study of stellar astrophysics and the structure of the Galaxy, andextragalactic astrophysics and cosmology (Zhao et al. 2012).”
• The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) (2012, methodology): “The pilot survey of LAMOST was launched on 2011 October 24 andfinished in 2012 June 24, as a test run of the whole system in survey mode in order to check t instrumental performance and assess the feasibility of the science goals of the LAMOST spectroscopic survey (Zhao et al. 2012).”
• 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.”