Contemporaneous optical-radio observations of a fast radio burst in a close galaxy pair

Open Access
Authors
  • K.Y. Hanmer
  • I. Pastor-Marazuela
  • J. Brink
  • D. Malesani
  • B.W. Stappers
  • P.J. Groot
  • A.J. Cooper
  • N. Tejos
  • D.A.H. Buckley
  • E.D. Barr
  • M.C. Bezuidenhout
  • S. Bloemen
  • M. Caleb
  • L.N. Driessen
  • R. Fender
  • F. Jankowski
  • M. Kramer
  • D.L.A. Pieterse
  • K.M. Rajwade
  • J. Tian
  • P.M. Vreeswijk
  • R. Wijnands
  • P.A. Woudt
Publication date 04-2025
Journal Monthly Notices of the Royal Astronomical Society
Volume | Issue number 538 | 3
Pages (from-to) 1800-1815
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract

We present the MeerKAT discovery and MeerLICHT contemporaneous optical observations of the fast radio burst (FRB) 20230808F, which was found to have a dispersion measure of DM = 653.2 ± 0.4 pc cm−3. FRB 20230808F has a scattering time-scale τs = 3.1 ± 0.1 ms at 1563.6 MHz, a rotation measure RM = 169.4 ± 0.2 rad m−2, and a radio fluence Fradio = 1.72 ± 0.01 Jy ms. We find no optical counterpart in the time immediately after the FRB, nor in the 3 months after the FRB during which we continued to monitor the field of the FRB. We set an optical upper flux limit in MeerLICHT’s q-band of 11.7 μJy for a 60 s exposure which started ∼3.4 s after the burst, which corresponds to an optical fluence, Fopt, of 0.039 Jy ms on a time-scale of ∼3.4 s. We obtain an estimate for the q−band luminosity limit of vLv ∼ 1.3 × 1043 erg s−1. We localize the burst to a close galaxy pair at a redshift of zspec = 0.3472 ± 0.0002. Our time delay of ∼3.4 s between the FRB arrival time and the start of our optical exposure is the shortest ever for an as yet non-repeating FRB, and hence the closest to simultaneous optical follow-up that exists for such an FRB.

Document type Article
Language English
Published at https://doi.org/10.1093/mnras/staf289
Other links https://www.scopus.com/pages/publications/105001177185
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