A fast radio burst in the direction of the Virgo cluster
Devansh Agarwal, Duncan R. Lorimer, Anastasia Fialkov, Keith W., Bannister, Ryan M. Shannon, Wael Farah, Shivani Bhandari, Jean-Pierre, Macquart, Chris Flynn, Giuliano Pignata, Nicolas Tejos, Benjamin Gregg,, Stefan Os{\l}owski, Kaustubh Rajwade, Mitchell B. Mickaliger

TL;DR
This study conducted a targeted search for faint fast radio bursts near the Virgo cluster, detected one burst, and used non-detections to constrain the faint-end of the FRB luminosity function, informing future surveys.
Contribution
It provides the first constraints on the faint-end slope and minimum luminosity of the FRB luminosity function using observations of a galaxy cluster.
Findings
Detected one FRB in 300 hours of observation near Virgo.
Non-detections constrain the faint-end slope to less than 1.52.
Minimum luminosity of FRBs is constrained to be above 2×10^{40} erg/s.
Abstract
The rate of fast radio bursts (FRBs) in the direction of nearby galaxy clusters is expected to be higher than the mean cosmological rate if intrinsically faint FRBs are numerous. In this paper, we describe a targeted search for faint FRBs near the core of the Virgo cluster using the Australian Square Kilometer Array Pathfinder telescope. During 300 hr of observations, we discovered one burst, FRB 180417, with dispersion measure DM cmpc. The FRB was promptly followed up by several radio telescopes for 27 h, but no repeat bursts were detected. An optical follow-up of FRB 180417 using the PROMPT5 telescope revealed no new sources down to an -band magnitude of 20.1. We argue that FRB 180417 is likely behind the Virgo cluster as the Galactic and intracluster DM contribution are small compared to the DM of the FRB, and there are no galaxies in the line of sight. The…
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