  We present a spectroscopically identified catalogue of 72 DA white dwarfs
from the LAMOST pilot survey. 35 are found to be new identifications after
cross-correlation with the Eisenstein et al. and Villanova catalogues. The
effective temperature and gravity of these white dwarfs are estimated by Balmer
lines fitting. Most of them are hot white dwarfs. The cooling times and masses
of these white dwarfs are estimated by interpolation in theoretical evolution
tracks. The peak of mass distribution is found to be $\sim$ 0.6 $M_\odot$ which
is consistent with prior work in the literature. The distances of these white
dwarfs are estimated using the method of Synthetic Spectral Distances. All of
these WDs are found to be in the Galactic disk from our analysis of space
motions. Our sample supports the expectation white dwarfs with high mass are
concentrated near the plane of Galactic disk
