Zobrazeno 1 - 10
of 96
pro vyhledávání: '"Kitaeva, M. A."'
Autor:
Tyul'bashev, S. A., Kitaeva, M. A., Pervoukhin, D. V., Tyul'basheva, G. E., Brylyakova, E. A., Chernosov, A. V., Ovchinnikov, I. L.
The search for rotating radio transients (RRAT) was done at a frequency of 111 MHz, in daily observations carried out on the radio telescope, a Large Phased Array (LPA) at declinations -9o < decj < +42o. 19 new RRATs were discovered for dispersion me
Externí odkaz:
http://arxiv.org/abs/2407.01285
Pushchino multibeams pulsar search. IV. Detection of new pulsars at declinations -9o < \delta < +55o
Autor:
Tyul'bashev, S. A., Tyul'basheva, G. E., Kitaeva, M. A., Ovchinnikov, I. L., Oreshko, V. V., Logvinenko, S. V.
The search for pulsars in monitoring data obtained at the radio telescope Large Phased Array (LPA) at a frequency of 111 MHz was carried out. Daily round-the-clock observations were carried out for about 3,000 days. The duration of the observation se
Externí odkaz:
http://arxiv.org/abs/2401.10706
Autor:
Tyul'bashev, S. A., Kitaeva, M. A., Brylyakova, E. A., Tyul'bashev, V. S., Tyul'basheva, G. E.
A search for pulsed radiation at a frequency of 111 MHz in the direction of 116 RRAT candidates was carried out. For the search, archival data obtained on a meridian 128-beam radio telescope, a Large Phased Array (LPA), was used. For each candidate,
Externí odkaz:
http://arxiv.org/abs/2401.05142
The effect of interplanetary plasma on pulsed pulsar radiation passing through is considered. The pulses of two rotating radio transients (J0609+16, J1132+25) and a pulsar (B0320+39) detected on the Large Phased Array (Pushchino observatory) were ana
Externí odkaz:
http://arxiv.org/abs/2305.07422
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 square degrees are explored. Despite repeated observations of the sam
Externí odkaz:
http://arxiv.org/abs/2208.04578
Publikováno v:
Astronomy Reports, 2020, V.64, Issue 5, p.406-424
The search for compact components of strong ($S_{int} \ge 5$ Jy at 102.5 MHz) discrete radio sources from the Pushchino catalogue was carried out using the method of interplanetary scintillation. A total of 3620 sources were examined, and 812 of them
Externí odkaz:
http://arxiv.org/abs/2207.07459
Autor:
Tyul'bashev, S. A., Tyul'bashev, V. S., Kitaeva, M. A., Chernyshova, A. I., Malofeev, V. M., Chashey, I. V., Shishov, V. I., Dagkesamanskii, R. D., Klimenko, S. V., Nikitin, I. N., Nikitina, L. D.
Publikováno v:
Astronomy Reports, 2017, V.61, pp.848-858
Pulsars with periods more than 0.4 seconds in the declination range -9o < decj < 42o and in the right ascension range 0h < r.a.< 24h were searched in parallel with the program of interplanetary scintillations monitoring of a large number of sources w
Externí odkaz:
http://arxiv.org/abs/2205.01960
Publikováno v:
Astronomy Reports, 2020, V.64, p.526
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 new pulsars were detected. Candidates into pulsars were selected in t
Externí odkaz:
http://arxiv.org/abs/2204.09489
Autor:
Tyul'bashev, S. A., Kitaeva, M. A.
Publikováno v:
Bulletin of the Lebedev Physics Institute, 2020, v.46, p.225
The search for radio emission from the gamma pulsar J0357+3205 in the meter wavelength range was carried out. Periodic emission was found in one of the 1,700 observation sessions. The average pulsar profile is single-component with a half-width of 20
Externí odkaz:
http://arxiv.org/abs/2204.07348
Publikováno v:
Astronomy Reports, 2021, V.65, p.819-825
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 known pulsar periods were found. The upper estimations of the integral f
Externí odkaz:
http://arxiv.org/abs/2204.06785