VizieR Online Data Catalog: M-type star magnetic activities from LAMOST & Kepler (Lu+, 2019)

LAMOST (also known as Guoshoujing Telescope), located in Xinglong Station of the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC), is a special meridian reflecting Schmidt telescope with about 4m effective aperture and a 5° field of view. LAMOST can obtain about 4000 spectra with a wavelength range of 3650-9000Å and a resolution R~1800 in one single exposure. The five-year regular survey ended on 2017 June 16, and all spectra were provided through the LAMOST DR5.

There are also some overlaps between the observation areas of the LAMOST and Kepler K2 missions. The Kepler spacecraft was equipped with a telescope with a 95cm aperture and 105deg² field of view.

(5 data files).