output
19952025
most citedFIRE5: a C++ implementation of Feynman Integral REduction

428 citations

Showing 2022 · astro-ph.HEShow all

6 papers · 2 filters

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★ 3 cited

Search for periodic emission of five gamma-ray pulsars at the frequency of 111 MHz

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

The search for pulsar (periodic) emission of five gamma-ray pulsars was carried out using the summed power spectra and the summed periodograms. No harmonics corresponding to the kn…

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…