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The High Time Resolution Universe survey-XIV. Discovery of 23 pulsars through GPU-accelerated reprocessing

  • V. Morello
  • , E. D. Barr
  • , S. Cooper
  • , M. Bailes
  • , S. Bates
  • , N. D.R. Bhat
  • , M. Burgay
  • , S. Burke-Spolaor
  • , A. D. Cameron
  • , D. J. Champion
  • , R. P. Eatough
  • , C. M.L. Flynn
  • , A. Jameson
  • , S. Johnston
  • , M. J. Keith
  • , E. F. Keane
  • , M. Kramer
  • , L. Levin
  • , C. Ng
  • , E. Petroff
  • A. Possenti, B. W. Stappers, W. Van Straten, C. Tiburzi
  • University of Manchester
  • Swinburne University of Technology
  • Max-Planck-Institut für Radioastronomie
  • Curtin University
  • Osservatorio Astronomico di Cagliari
  • West Virginia University
  • Commonwealth Scientific Industrial and Research Organization
  • University of British Columbia
  • University of Amsterdam
  • Cagliari State University
  • Auckland University of Technology
  • Bielefeld University

Research output: Contribution to a Journal (Peer & Non Peer)Articlepeer-review

77 Citations (Scopus)

Abstract

We have performed a new search for radio pulsars in archival data of the intermediate and high Galactic latitude parts of the Southern High Time Resolution Universe pulsar survey. This is the first time the entire dataset has been searched for binary pulsars, an achievement enabled by GPU-accelerated dedispersion and periodicity search codes nearly 50 times faster than the previously used pipeline. Candidate selection was handled entirely by a Machine Learning algorithm, allowing for the assessment of 17.6 million candidates in a few persondays. We have also introduced an outlier detection algorithm for efficient radio-frequency interference (RFI) mitigation on folded data, a new approach that enabled the discovery of pulsars previously masked by RFI. We discuss implications for future searches, particularly the importance of expanding work on RFI mitigation to improve survey completeness. In total, we discovered 23 previously unknown sources, including 6 millisecond pulsars and at least 4 pulsars in binary systems. We also found an elusive but credible redback candidate that we have yet to confirm.

Original languageEnglish
Pages (from-to)3673-3685
Number of pages13
JournalMonthly Notices of the Royal Astronomical Society
Volume483
Issue number3
DOIs
Publication statusPublished - 1 Mar 2019
Externally publishedYes

Keywords

  • Methods: data analysis
  • Pulsars: general

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