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

Journal Article · · Monthly Notices of the Royal Astronomical Society
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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 $$\mathrm{DM}=653.2\pm 0.4\mathrm{\, pc\, cm^{-3}}$$. FRB 20230808F has a scattering time-scale $$\tau _{s}=3.1\pm 0.1\, \mathrm{ms}$$ at 1563.6 MHz, a rotation measure $$\mathrm{RM}=169.4\pm 0.2\, \mathrm{rad\, m^{-2}}$$, and a radio fluence $$F_{\mathrm{radio}}=1.72\pm 0.01\, \mathrm{Jy\, ms}$$. 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 $$11.7\, \mathrm{\mu Jy}$$ for a 60 s exposure which started $${\sim}3.4$$ s after the burst, which corresponds to an optical fluence, $$F_{\mathrm{opt}}$$, of $$0.039\, \mathrm{Jy\, ms}$$ on a time-scale of $${\sim}3.4$$ s. We obtain an estimate for the $q-$band luminosity limit of $$vL_{v}\sim 1.3\times 10^{43}\, \mathrm{erg\, s^{-1}}$$. We localize the burst to a close galaxy pair at a redshift of $$z_{\mathrm{spec}}=0.3472\pm 0.0002$$. Our time delay of $${\sim}3.4$$ 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.

Sponsoring Organization:
USDOE
OSTI ID:
2536749
Journal Information:
Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 3 Vol. 538; ISSN 0035-8711
Publisher:
Oxford University PressCopyright Statement
Country of Publication:
United Kingdom
Language:
English

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