A fast radio burst with a low dispersion measure

E. Petroff, L. C. Oostrum, B. W. Stappers, M. Bailes, E. D. Barr, S. Bates, S. Bhandari, 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, E. F. Keane, M. J. Keith, M. Kramer, L. LevinV. Morello, C. Ng, A. Possenti, V. Ravi, W. Van Straten, D. Thornton, C. Tiburzi

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

24 Citations (Scopus)

Abstract

Fast radio bursts (FRBs) are millisecond pulses of radio emission of seemingly extragalactic origin. More than 50 FRBs have now been detected, with only one seen to repeat. Here we present a new FRB discovery, FRB 110214, which was detected in the high-latitude portion of the High Time Resolution Universe South survey at the Parkes telescope. FRB 110214 has one of the lowest dispersion measures of any known FRB (DM = 168.8 ± 0.5 pc cm-3), and was detected in two beams of the Parkes multibeam receiver. A triangulation of the burst origin on the sky identified three possible regions in the beam pattern where it may have originated, all in sidelobes of the primary detection beam. Depending on the true location of the burst the intrinsic fluence is estimated to fall in the range of 50-2000 Jy ms, making FRB 110214 one of the highest fluence FRBs detected with the Parkes telescope. No repeating pulses were seen in almost 100 h of follow-up observations with the Parkes telescope down to a limiting fluence of 0.3 Jy ms for a 2 ms pulse. Similar low DM, ultrabright FRBs may be detected in telescope sidelobes in the future, making careful modelling of multibeam instrument beam patterns of utmost importance for upcoming FRB surveys.

Original languageEnglish
Pages (from-to)3109-3115
Number of pages7
JournalMonthly Notices of the Royal Astronomical Society
Volume482
Issue number3
DOIs
Publication statusPublished - 2019
Externally publishedYes

Keywords

  • Methods: data analysis
  • galaxies: statistics
  • radio continuum: transients

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