  We present an ongoing survey with the Nan\c{c}ay Radio Telescope at L-band.
The targeted area is $74^\circ \lesssim l <150^\circ$ and $3.5^\circ < |b| <
5^\circ$. This survey is characterized by a long integration time (18 min),
large bandwidth (512 MHz) and high time and frequency resolution (64 $\mu$s and
0.5 MHz) giving a nominal sensitivity limit of 0.055 mJy for long period
pulsars. This is about 2 times better than the mid-latitude HTRU survey, and is
designed to be complementary with current large scale surveys. This survey will
be more sensitive to transients (RRATs, intermittent pulsars), distant and
faint millisecond pulsars as well as scintillating sources (or any other kind
of radio faint sources) than all previous short-integration surveys.
