Pushchino multibeams pulsar search. IV. Detection of new pulsars at declinations -9o < \delta < +55o

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 session for each direction in the sky was 3.5 minute...

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Bibliographic Details
Published in:arXiv.org 2024-01
Main Authors: Tyul'bashev, S A, Tyul'basheva, G E, Kitaeva, M A, Ovchinnikov, I L, Oreshko, V V, Logvinenko, S V
Format: Article
Language:English
Subjects:
Phased arrays
Power spectra
Pulsars
Radio telescopes
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Summary: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 session for each direction in the sky was 3.5 minutes per day. The search for pulsars was carried out using power spectra. To search for weak pulsars, power spectra were summed up. The expected increase in sensitivity was 35-40 times compared to observations in one session. In a blind search, 330 pulsars with regular radiation were detected, with periods (P) from 0.0333 to 3.7455 s and dispersion measures (DM) up to 249 pc/cm3. 39 pulsars turned out to be new. Average profiles were obtained for 6 pulsars. The DM for 7 pulsars previously detected on the LPA have been clarified.
ISSN:2331-8422
DOI:10.48550/arxiv.2401.10706