S. A. Tyul'bashev, M. A. Kitaeva, S. V. Logvinenko, G. E. Tyul'basheva
Published 2022-04-11Version 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 detected. More then 80% of these sources are known pulsars observed in the side lobes of the antenna. From one to several hundreds pulses were detected in twelve known pulsars. For four pulsars (J0157+6212, J1910+5655, J2337+6151, J2354+6155) the narrowness of the strongest pulses and the ratio of peak flux densities in the strongest pulse and in the average profile indicate that they can be pulsars with giant pulses. One new rotating radio transient (RRAT) J0812+8626 with a dispersion measure DM=40.25 pc/cm3 was detected.
Comments: Published in Astronomy Reports and translated from russian version of paper by Yandex translator with correction scientific lexis. 6 page, 4 figures, 1 table
Journal: Astronomy Reports, 2021, v.65, p.1246
Pushchino multibeams pulsar search. IV. Detection of new pulsars at declinations -9o < δ< +55o
Detection of Five New RRATs at 111 MHz
Detection Statistics of Pulse Signals at Declinations from $+42^o$ to $+52^o$ at the Frequency 111 MHz
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