  On the Large Phased Array (LPA) of Lebedev Physics Institute (LPI), a search
for pulsars outside the Galaxy plane was carried out in a 300 sq. deg area. The
search with a sensitivity 5-10 times better than that of previously conducted
surveys was at a frequency of 111 MHz. The search was carried out in the summed
power spectra. With an accumulation equivalent to 100 hours of continuous
observations for each point of the area, 5 known pulsars were detected with a
signal-to-noise ratio (S/N) from 20 to 1300 in the first harmonic of the
spectrum. Average profiles were obtained for the detected pulsars. Estimates of
the peak and integral flux densities of the found pulsars are given for
individual sessions and for the power spectra summarized over 5.5 years,
obtained using the developed method based on measurements of the height of
harmonics in the power spectrum. No new pulsars have been detected in the area.
Apparently, when searching for pulsars in the area, we have approached the
lower limit of the luminosity of the second pulsars. The completeness of the
survey is at the level of 0.5 mJy.
