000004099 001__ 4099
000004099 005__ 20190204145043.0
000004099 037__ $$aSEMIN-2019-0015
000004099 100__ $$aDe Cat, P.
000004099 245__ $$aThe LAMOST-Kepler project: past, present, and future
000004099 260__ $$c2018
000004099 269__ $$c2018-12-14
000004099 520__ $$aThe Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) is a unique instrument located at the Xinglong observatory (China) that combines a large aperture (4-m telescope) with a wide field of view (circular region with a diameter of 5 degrees on the sky) that is covered with 4000 optical fibers. It is the ideal tool to obtain low/medium-resolution spectra (R~1800/7500) for a large number of objects in an efficient way. The LAMOST-Kepler project was initiated in 2009 with the main aim to gather LAMOST spectra for as many objects as possible in the field-of-view of the Kepler space mission to allow a homogeneous spectroscopic determination of the basic stellar parameters of the observed stars. In this review talk, the past, present and future activities within the LAMOST-Kepler consortium will be discussed in which the importance of the LAMOST-Kepler observations will be highlighted. What could be the role of LAMOST for the current and future space missions?
000004099 536__ $$aBL/$$c33/$$fFWI20 
000004099 594__ $$aNO
000004099 700__ $$aLAMOST-Kepler, consortium
000004099 773__ $$tBeijing Normal University (BNU), Beijing, China
000004099 8560_ $$fpeter.decat@observatoire.be
000004099 8564_ $$s26533520$$uhttps://publi2-as.oma.be/record/4099/files/Seminar_PeterDeCat_2018_Beijing.pdf
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000004099 8564_ $$s12368$$uhttps://publi2-as.oma.be/record/4099/files/Seminar_PeterDeCat_2018_Beijing.jpg?subformat=icon-180$$xicon-180
000004099 980__ $$aSEMIN