Detection of Five New RRATs at 111 MHz

Abstract

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-four pulsating sources were detected at declinations $-9^o<\delta <+42^o$. Forty-seven of these are known pulsars, five are new sources, and two are previously discovered transients. Estimates of the peak flux densities and dispersion measures are presented or all these sources.

arXiv commentpublished in Astronomy Report, translated by Yandex translator with correction of scientific lexis, 8 pages, 2 figures, 3 tables

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Cited by in corpus (21)

• The FAST Galactic Plane Pulsar Snapshot Survey: II. Discovery of 76 Galactic rotating radio transients and their enigma
• Detection of 25 new rotating radio transients at 111 MHz
• Pushchino multibeam pulsar search: I. Targeted search of weak pulsars
• Search for pulsars in the summed power spectra at a frequency of 111 MHz
• Pulse energy distribution for RRAT J0139+33 according to observations at the frequency 111 MHz
• Detection of two new RRATs at 111 MHz
• Detection Statistics of Pulse Signals at Declinations from $+42^o$ to $+52^o$ at the Frequency 111 MHz
• Investigation of four rotating radio transients properties at 111 MHz
• Pushchino multibeam pulsar search -- II. Long-term variability of RRATs
• The second decametre pulsar census at UTR-2 radio telescope
• Pushchino multibeams pulsar search. IV. Detection of new pulsars at declinations -9o < δ< +55o
• Revisiting Pushchino RRAT search using neural network
• Search for Dispersed Pulses at Declinations from +56o to +87o
• Detection of two new RRATs at 111 MHz
• Search for fast radio transients using Arecibo drift-scan observations at 1.4 GHz
• Polarized radio emission of RRAT J1854+0306
• Interplanetary scintillation and pulsar pulse statistics
• Peculiarities of radio emission from new pulsars at 111 MHz
• Study of the variability and components of the pulsar B0823+26 at a frequency of 111 MHz
• Pulsars identified in the LOFAR Two-metre Sky Survey at 144 MHz
• Pushchino multibeams pulsar search -- III. Drift periods of pulsars from summed power spectra method