  The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) at the
Xinglong observatory in China is a new 4-m telescope equipped with 4,000
optical fibers. In 2010, we initiated the LAMOST-Kepler project. We requested
to observe the full field-of-view of the nominal Kepler mission with the LAMOST
to collect low-resolution spectra for as many objects from the KIC10 catalogue
as possible. So far, 12 of the 14 requested LAMOST fields have been observed
resulting in more than 68,000 low-resolution spectra. Our preliminary results
show that the stellar parameters derived from the LAMOST spectra are in good
agreement with those found in the literature based on high-resolution
spectroscopy. The LAMOST data allows to distinguish dwarfs from giants and can
provide the projected rotational velocity for very fast rotators.
