  The nearly continuous light curves with micromagnitude precision provided by
the space mission Kepler are revolutionising our view of pulsating stars. They
have revealed a vast sea of low-amplitude pulsation modes that were
undetectable from Earth. The long time base of Kepler light curves allows an
accurate determination of frequencies and amplitudes of pulsation modes needed
for in-depth asteroseismic modeling. However, for an asteroseismic study to be
successful, the first estimates of stellar parameters need to be known and they
can not be derived from the Kepler photometry itself. The Kepler Input Catalog
(KIC) provides values for the effective temperature, the surface gravity and
the metallicity, but not always with a sufficient accuracy. Moreover,
information on the chemical composition and rotation rate is lacking. We are
collecting low-resolution spectra for objects in the Kepler field of view with
the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST, Xinglong
observatory, China). All of the requested fields have now been observed at
least once. In this paper we describe those observations and provide a database
of use to the whole astronomical community.
