Detection of Five New Pulsars with the BSA LPI Radio Telescope

Autor:	M. A. Kitaeva, V. M. Malofeev, G. E. Tyul’basheva, S. A. Tyul’bashev, V. S. Tyul’bashev
Rok vydání:	2020
Předmět:	Physics 010308 nuclear & particles physics Astrophysics::High Energy Astrophysical Phenomena Astronomy and Astrophysics Astrophysics 01 natural sciences Declination Galaxy Spectral line Radio telescope Noise generator Pulsar Space and Planetary Science 0103 physical sciences 010303 astronomy & astrophysics
Zdroj:	Astronomy Reports. 64:526-532
ISSN:	1562-6881 1063-7729
DOI:	10.1134/s1063772920060074
Popis:	During five years of daily observations, the search for new pulsars using the BSA LPI radio telescope in 96 spatial beams covering 17 000 square degrees was conducted. Five new pulsars were identified. Candidate pulsars were selected in summed power spectra. A noise generator was used to renormalize data and total the power spectra for individual directions correctly. As a result, the sensitivity increased by a factor of 10–20 relative to that in individual observational sessions. The sensitivity for pulsars with pulses longer than 100 ms at declinations +30° < δ < +40° was 1.2 and 0.4 mJy in and out of the galaxy plane, respectively.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::58662b2c37f4d0c35d085817c4cb526b https://doi.org/10.1134/s1063772920060074 Zobrazit plný text záznamu Plný text ve formátu PDF Plný text ve formátu HTML
Nepřihlášeným uživatelům se plný text nezobrazuje	K zobrazení výsledku je třeba se přihlásit.