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Detection of new pulsars at the frequency 111 MHz
S. A. Tyul'bashev, V. S. Tyul'bashev, V. V. Oreshko +1
The pulsar search was started at the radio telescope LPA LPI at the frequency 111~MHz. The first results deals of a search for right ascension and declinations $+21^{\…
Detection of Five New RRATs at 111 MHz
S. A. Tyul'bashev, V. S. Tyul'bashev, V. M. Malofeev +6
Results of 111-MHz monitoring observations carried out on the Big Scanning Antenna of the Pushchino Radio Astronomy Observatory during September 1-28, 2015 are presented. Fifty-fou…
Detection Statistics of Pulse Signals at Declinations from to at the Frequency 111 MHz
V. A. Samodurov, S. A. Tyul'bashev, M. O. Toropov +1
A search for pulse signals was carried out in a new sky area included in the monitoring program for the search for pulsars and transients. Processing of several months data recorde…
Detection of two new RRATs at 111 MHz
S. V. Logvinenko, S. A. Tyul'bashev, V. M. Malofeev
Two new rotating transients were detected in the 2020 observations carried out on the LPA LPI radio telescope. The dispersion measures of the found transients are DM=21 and 35 pc/c…
Search for Dispersed Pulses at Declinations from +56o to +87o
S. A. Tyul'bashev, M. A. Kitaeva, S. V. Logvinenko +1
The survey of northern hemisphere were made at a frequency of 111 MHz. The total accumulation time at each point of the sky was at least one hour. 75 sources of pulse emission were…
Pushchino multibeam pulsar search -- II. Long-term variability of RRATs
T. V. Smirnova, S. A. Tyul'bashev, E. A. Brylyakova +5
Pulses from 16 previously known rotating radio transients (RRAT) have been searched at the 110 MHz daily monitor program for 4 to 5.5 years by using the Large-Phased-Array (LPA) at…