Detection of Five New RRATs at 111 MHz

S. A. Tyul’bashev; V. S. Tyul’bashev; V. M. Malofeev; S. V. Logvinenko; V. V. Oreshko; R. D. Dagkesamanskii; I. V. Chashei; V. I. Shishov; N. N. Bursov

doi:10.1134/S1063772918010079

Detection of Five New RRATs at 111 MHz

Авторы: Tyul’bashev S.A.¹, Tyul’bashev V.S.¹, Malofeev V.M.¹, Logvinenko S.V.¹, Oreshko V.V.¹, Dagkesamanskii R.D.¹, Chashei I.V.¹, Shishov V.I.¹, Bursov N.N.²
Учреждения:
1. Pushchino Radio Astronomy Observatory, Astro Space Center
2. Special Astrophysical Observatory
Выпуск: Том 62, № 1 (2018)
Страницы: 63-71
Раздел: Article
URL: https://ogarev-online.ru/1063-7729/article/view/191394
DOI: https://doi.org/10.1134/S1063772918010079
ID: 191394

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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° < δ < 42°. Forty-seven of these are known pulsars, five are new sources, and two are previously discovered transients. Estimates of the peak flux densities and dispersion measures are presented for all these sources.