  The search of pulsars in monitoring observations being carried out for 5
years using LPA LPI radio telescope was done in 96 spatial beams covering daily
17,000 square degrees. Five new pulsars were detected. Candidates into pulsars
were selected in the summed power spectra. The use of a noise generator allowed
to renormalize the data and to perform correct summing up of the power spectra
for individual directions in the sky. Herewith, the sensitivity increased more
than 20 times in comparison with individual sessions of observations. For
pulsars with pulse durations greater than 100 ms at declinations +30o<dec.<+40o
it is equal to 1.2 mJy and 0.4 mJy in/out of the Galaxy plane.
