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20222026
most citedPushchino multibeam pulsar search: I. Targeted search of weak pulsars

30 citations · 91 across the 16 of their papers we have counts for

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6 papers · 1 filter

astro-ph.HE2022★ 2 cited

Pushchino multibeams pulsar search. First results

S. A. Tyul'bashev, G. E. Tyul'basheva, M. A. Kitaeva

Since the discovery of pulsars, dozens of surveys have already been conducted with their searches. In the course of surveys in the sky, areas from thousands to tens of thousands of…

astro-ph.HE2022★ 19 cited

Search for pulsars in the summed power spectra at a frequency of 111 MHz

S. A. Tyul'bashev, M. A. Kitaeva, V. S. Tyul'bashev +2

The search of pulsars in monitoring observations being carried out for 5 years using LPA LPI radio telescope was done in 96 spatial beams covering daily 17,000 square degrees. Five…

astro-ph.HE2022★ 6 cited

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…

astro-ph.HE2022★ 8 cited

Revisiting Pushchino RRAT search using neural network

S. A. Tyul'bashev, D. V. Pervukhin, M. A. Kitaeva +3

The search for rotating radio transients (RRAT) at declination from -9o to +42o was carried out in the semi-annual monitoring data obtained on the Large Phased Array (LPA) radio te…

astro-ph.HE2022★ 30 cited

Pushchino multibeam pulsar search: I. Targeted search of weak pulsars

S. A. Tyul'bashev, M. A. Kitaeva, G. E. Tyul'basheva

The search for pulsars in a sample of pulsar candidates found based on a multi-year survey conducted with low (6 channels; sampling 0.1s) time-frequency resolution on declinations…

astro-ph.HE2022★ 10 cited

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…