Detection of new pulsars at 111 MHz
- Authors: Tyul’bashev S.A.1, Tyul’bashev V.S.2, Oreshko V.V.1, Logvinenko S.V.1
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Affiliations:
- Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
- Lomonosov Moscow State University
- Issue: Vol 60, No 2 (2016)
- Pages: 220-232
- Section: Article
- URL: https://bakhtiniada.ru/1063-7729/article/view/189701
- DOI: https://doi.org/10.1134/S1063772916020128
- ID: 189701
Cite item
Abstract
The first results of a search for pulsars using the Large Phased Array of the Lebedev Physical Institute at 111 MHz for right ascensions 0h-24h and declinations 21°-42° are reported. Data with a time resolution of 100 ms in six frequency channels within a 2.5-MHz frequency band have been processed. Thirty-four pulsars have been detected, of which seventeen were observed on this telescope earlier; ten known pulsars had not been observed earlier. Seven new pulsars have been discovered.
About the authors
S. A. Tyul’bashev
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Author for correspondence.
Email: serg@prao.ru
Russian Federation, Pushchino, Moscow oblast, 142290
V. S. Tyul’bashev
Lomonosov Moscow State University
Email: serg@prao.ru
Russian Federation, Moscow, 119991
V. V. Oreshko
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Email: serg@prao.ru
Russian Federation, Pushchino, Moscow oblast, 142290
S. V. Logvinenko
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Email: serg@prao.ru
Russian Federation, Pushchino, Moscow oblast, 142290
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