A fast radio burst with a low dispersion measure
| 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 |
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| 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.
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| 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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107.05 — A fast radio burst with a low dispersion
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