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The SUrvey for Pulsars and Extragalactic Radio Bursts V: Recent Discoveries and Full Timing Solutions

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arxiv 2006.13637 v1 pith:6KRLZHR2 submitted 2020-06-24 astro-ph.HE

R. Spiewak , C. Flynn , S. Johnston , E. F. Keane , M. Bailes , E. D. Barr , S. Bhandari , M. Burgay
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F. Jankowski M. Kramer V. Morello A. Possenti V. Venkatraman Krishnan
This is my paper · ORCID
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keywords pulsarsdiscoveriespulsarradiotimingburstsextragalacticparkes
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The SUrvey for Pulsars and Extragalactic Radio Bursts ran from 2014 April to 2019 August, covering a large fraction of the southern hemisphere at mid- to high-galactic latitudes, and consisting of 9-minute pointings taken with the 20-cm multibeam receiver on the Parkes Radio Telescope. Data up to 2017 September 21 have been searched using standard Fourier techniques, single-pulse searches, and Fast Folding Algorithm searches. We present 19 new discoveries, bringing the total to 27 discoveries in the programme, and we report the results of follow-up timing observations at Parkes for 26 of these pulsars, including the millisecond pulsar PSR J1421-4409; the faint, highly-modulated, slow pulsar PSR J1646-1910; and the nulling pulsar PSR J1337-4441. We present new timing solutions for 23 pulsars, and we report flux densities, modulation indices, and polarization properties.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 13 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. Unlocking the hidden potential of pulsar astronomy

    astro-ph.IM 2025-06 conditional novelty 3.0 of 10

    This review and feasibility study shows that compact radio receivers can detect bright pulsars for navigation, timing, randomness, and space weather applications, with a 4-meter dish potentially achieving 10 km self-l...

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