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Using five year monitoring observations, we did a blind search for pulses forrotating radio transient (RRAT) J0139+33 and PSR B0320+39. At the interval \pm1.5m of the time corresponding to the source passing through the meridian, wedetected 39377 individual pulses for the pulsar B0320+39 and 1013 pulses forRRAT J0139+33. The share of registered pulses from the total number of observedperiods for the pulsar B0320+39 is 74%, and for the transient J0139+33 it is0.42%. Signal-to-noise ratio (S/N) for the strongest registered pulses isapproximately equal to: S/N = 262 (for B0320+39) and S/N = 154 (for J0139+33).  Distributions of the number of detected pulses in S/N units for the pulsarand for the rotating transient are obtained. The distributions could beapproximated with a lognormal and power dependencies. For B0320+39 pulsar, thedependence is lognormal, it turns into a power dependence at high values ofS/N, and for RRAT J0139+33, the distribution of pulses by energy is describedby a broken (bimodal) power dependence with an exponent of about 0.4 and 1.8(S/N < 19 and S/N > 19).  We have not detected regular (pulsar) emission of J0139+33. Analysis of theobtained data suggests that RRAT J0139+33 is a pulsar with giant pulses.

Pulse energy distribution for RRAT J0139+33 according to observations at the frequency 111 MHz