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The search for pulsars in monitoring data obtained at the radio telescopeLarge Phased Array (LPA) at a frequency of 111 MHz was carried out. Dailyround-the-clock observations were carried out for about 3,000 days. Theduration of the observation session for each direction in the sky was 3.5minutes per day. The search for pulsars was carried out using power spectra. Tosearch for weak pulsars, power spectra were summed up. The expected increase insensitivity was 35-40 times compared to observations in one session. In a blindsearch, 330 pulsars with regular radiation were detected, with periods (P) from0.0333 to 3.7455 s and dispersion measures (DM) up to 249 pc/cm3. 39 pulsarsturned out to be new. Average profiles were obtained for 6 pulsars. The DM for7 pulsars previously detected on the LPA have been clarified.

Pushchino multibeams pulsar search. IV. Detection of new pulsars at declinations -9o < \delta < +55o