A fast radio burst with a low dispersion measure

Open Access
Authors
Publication date 01-2019
Journal American Astronomical Society Meeting
Event 233rd Meeting of the American Astronomical Society
Article number 107.05
Volume | Issue number 233
Pages (from-to) 15
Number of pages 1
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
Fast radio bursts (FRBs) are millisecond pulses of radio emission of seemingly extragalactic origin. More than 35 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 = 168.9$\pm$0.5 pc cm$^{-3}$), and was detected in two beams of the Parkes multi-beam 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 to date. No repeating pulses were seen in almost 100 hours 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, ultra-bright FRBs may be detected in telescope sidelobes in the future, making careful modeling of multi-beam instrument beam patterns of utmost importance for upcoming FRB surveys.
Document type Meeting Abstract
Language English
Published at https://assets.pubpub.org/qmxqtups/61582749069276.pdf
Other links https://ui.adsabs.harvard.edu/abs/2019AAS...23310705P/abstract
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