Zobrazeno 1 - 10
of 87
pro vyhledávání: '"Logvinenko, S. V."'
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:
Samodurov, V. A., Tyul'bashev, S. A., Toropov, M. O., Dolgushev, A. V., Oreshko, V. V., Logvinenko, S. V.
Publikováno v:
Astronomy Reports, 2023, Vol. 67, p. 590-595
A search for pulse signals in a area with declinations of $+52\degr <\delta <+55\degr$ was carried out on the LPA LPI radio telescope. When processing ten months of observations recorded in six frequency channels with a channel width of 415 kHz and a
Externí odkaz:
http://arxiv.org/abs/2309.00845
Publikováno v:
Astronomy Reports, 2016, v.60, p.220
The pulsar search was started at the radio telescope LPA LPI at the frequency 111~MHz. The first results deals of a search for right ascension $0^h - 24^h$ and declinations $+21^{\circ} - +42^{\circ}$ are presented in paper. The data with sampling 10
Externí odkaz:
http://arxiv.org/abs/2208.08839
Autor:
Tyul'bashev, S. A., Tyul'bashev, V. S., Malofeev, V. M., Logvinenko, S. V., Oreshko, V. V., Dagkesamanskii, R. D., Chashei, I. V., Shishov, V. I., Bursov, N. N.
Publikováno v:
Astronomy Reports, 2018, V.62, Issue 1, pp.63-71
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
Externí odkaz:
http://arxiv.org/abs/2207.11032
Publikováno v:
Astronomy Reports, 2022, V.66, Issue 4, p.341-347
A search for pulse signals was carried out in a new sky area included in the monitoring program for the search for pulsars and transients. Processing of several months data recorded in six frequency channels with a total bandwidth of 2.5 MHz showed t
Externí odkaz:
http://arxiv.org/abs/2207.09197
Publikováno v:
Bulletin of the Lebedev Physics Institute, 2020, vol. 47, issue 12, pp. 390-393
Two new rotating transients were detected in the 2020 observations carried out on the LPA LPI radio telescope. The dispersion measures of the found transients are DM=21 and 35 pc/cm^3, the pulse half-widths are We=18 and 35 ms for J1550+09 and J2047+
Externí odkaz:
http://arxiv.org/abs/2206.12108
Publikováno v:
Astronomy Reports, 2021, v.65, p.1246
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 detected. More then 80% of these sources are known pulsars observed i
Externí odkaz:
http://arxiv.org/abs/2204.04933
Autor:
Smirnova, T. V., Tyul'bashev, S. A., Brylyakova, E. A., Kitaeva, M. A., Chashei, I. V., Tyul'basheva, G. E., Oreshko, V. V., Logvinenko, S. V.
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 Pushchino. The total number of pulses detected in such a long observa
Externí odkaz:
http://arxiv.org/abs/2203.13597
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.