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

Using five-year-monitoring observations, we carried out a blind search for pulses rotating radio transient (RRAT) J0139+33 and PSR B0320+39. At the interval ±1.5 m of time corresponding to source passing through meridian, detected 39377 individual pulsar B0320+39 1013 RRAT J0139+33. The share registered from total number observed periods is 74%, it 0.42%. signal-to-noise ratio (S/N) strongest is, approximately, following: S / N = 262 (for B0320+39) 154 J0139+33). We obtained distributions in S/N units transient. could be approximated with lognormal power dependences. For pulsar, dependence lognormal, turns into at high values S/N; J0139+33, distribution by energy described broken (bimodal) an exponent about 0.4 1.8 ( ≤ 19 ≥ 19). did not detect regular (pulsar) emission Analysis data suggests that giant pulses.