  We present a sample of quasars discovered in the area of Galactic Anti-Center
(GAC) of $150^{\circ} \leq l \leq 210^{\circ}$ and $|b| \leq 30^{\circ}$, based
on the LAMOST Data Release 3 (DR3). The sample contains 151 spectroscopically
confirmed quasars. Among them 80 are newly discovered with the LAMOST. All
those quasars are very bright, with $i$ magnitudes peaking around 17.5\, mag.
All the newly quasars are discovered serendipitously, targeted originally with
the LAMOST as stars of bluer colours, except for a few targeted as variable,
young stellar object candidates. This bright quasar sample at low Galactic
latitudes will help fill the gap in the spatial distribution of known quasars
near the Galactic disk that are used to construct astrometric reference frame
for the purpose of accurate proper motion measurements, for example, Gaia. They
are also excellent tracers to probe the kinematics and chemistry of the
interstellar medium of the Milky Way disk and halo via absorption line
spectroscopy.
