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Search and detection of pulsars in the monitoring observations at the frequency 111 MHz

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arxiv 2205.01960 v1 pith:VQRI62MS submitted 2022-05-04 astro-ph.HE

classification astro-ph.HE
keywords pulsarsfrequencyobservationswereresolutioncandidateschannelsmonitoring
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Pulsars with periods more than 0.4 seconds in the declination range -9o < decj < 42o and in the right ascension range 0h < r.a.< 24h were searched in parallel with the program of interplanetary scintillations monitoring of a large number of sources with the radiotelescope LPA LPI. Four-year observations carried out at the central frequency 110.25 MHz in the band 2.5 MHz and in six frequency channels with the time resolution 100 ms were used for the search. Initial detections of candidates for pulsars were based on the Fourier power spectra averaged over the whole observations period. The candidates for pulsars were checked in more details from observations analysis with higher time-frequency resolution: 32 frequency channels with time resolution of 12.5 ms. 18 new pulsars was discovered, their main characteristics are presented.

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 29 citations worldwide. Full citation record

  1. FAST Pulsar Database III. Snapshots of nulling, mode-changing and subpulse modulation of 374 pulsars

    astro-ph.HE 2026-07 accept novelty 7.0 of 10

    Sensitive FAST L-band single-pulse sequences detect nulling, mode-changing or subpulse modulation in 374 pulsars, with hundreds of first reports and statistical links to older, longer-period, lower-Ė objects.

  2. Exploring the Magnetic Field Structure of the Milky Way with Pulsars in the SKA Era

    astro-ph.HE 2026-07 accept novelty 2.5 of 10

    SKA1 AA* and AA4 will roughly double-to-triple the known pulsar population and supply thousands of new RMs, enabling detailed 3D mapping of Galactic disk and halo magnetic fields.

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