  Using five year monitoring observations, we did a blind search for pulses for
rotating radio transient (RRAT) J0139+33 and PSR B0320+39. At the interval \pm
1.5m of the time corresponding to the source passing through the meridian, we
detected 39377 individual pulses for the pulsar B0320+39 and 1013 pulses for
RRAT J0139+33. The share of registered pulses from the total number of observed
periods for the pulsar B0320+39 is 74%, and for the transient J0139+33 it is
0.42%. Signal-to-noise ratio (S/N) for the strongest registered pulses is
approximately 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 pulsar
and for the rotating transient are obtained. The distributions could be
approximated with a lognormal and power dependencies. For B0320+39 pulsar, the
dependence is lognormal, it turns into a power dependence at high values of
S/N, and for RRAT J0139+33, the distribution of pulses by energy is described
by 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 the
obtained data suggests that RRAT J0139+33 is a pulsar with giant pulses.
