activity
20042025
most citedHard X-ray Emission Clumps in the gamma-Cygni Supernova Remnant: an INTEGRAL-ISGRI View

17 citations · 21 across the 6 of their papers we have counts for

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5 papers · 1 filter

astro-ph.HE2025

A nearby pulsar J1951+2837 observed by the LPA and FAST

T. V. Smirnova, D. J. Zhou, M. A. Kitaeva +5

PSR J1951+2837 is a nearby pulsar with a period of 7.334 s and dispersion measure of DM = 2.9 0.6 pc cm, located about 200 or 300 pc from the Sun. It occasionally radi…

astro-ph.HE2025★ 2 cited

Variations in the Radiation Intensity of Pulsar B0950+08: Nine Years of Monitoring at 110 MHz

T. V. Smirnova, M. O. Toropov, S. A. Tyul'bashev

The analysis of variations in the emission intensity of the pulsar B0950+08 from 2014 to 2022 with scales from minutes to years was carried out. The observations were obtained in a…

astro-ph.HE2025★ 1 cited

Search for weak components in pulsar radiation

T. V. Smirnova, M. O. Toropov, S. A. Tyul'bashev

The search for weak components outside the main pulse (MP) in the radiation of pulsars at a frequency of 110 MHz observed on the LPA LPI telescope in the Pushchino Multibeam Pulsar…

astro-ph.HE2024

Pushchino multibeams pulsar search -- III. Drift periods of pulsars from summed power spectra method

T. V. Smirnova, S. A. Tyul'bashev, M. A. Kitaeva +1

The drift periods P2 and P3 were searched for using the summed power spectra of 41 pulsars observed at declinations from -9o to +42o. The power spectra of pulses with a given perio…

astro-ph.HE2023★ 1 cited

Study of the variability and components of the pulsar B0823+26 at a frequency of 111 MHz

M. O. Toropov, S. A. Tyul'bashev, T. V. Smirnova +2

Studies of the pulsar B0823+26 have been carried out using the Large Phased Array (LPA) radio telescope. At time span of 5.5 years, the amplitudes of the main pulse (MP), postcurso…