A Demonstration of Extremely Low Latency $\gamma$-ray, X-Ray & UV Follow-Up of a Millisecond Radio Transient
Aaron Tohuvavohu, Casey J. Law, Jamie A. Kennea, Elizabeth A. K., Adams, Kshitij Aggarwal, Geoffrey Bower, Sarah Burke-Spolaor, Bryan J., Butler, John M. Cannon, S. Bradley Cenko, James DeLaunay, Paul Demorest,, Maria R. Drout, Philip A. Evans, Alec S. Hirschauer, T. J. W. Lazio

TL;DR
This paper demonstrates a novel, ultra-low latency follow-up observation of a potential Fast Radio Burst using Swift, achieving over ten times faster response than previous efforts, but no coincident high-energy emission was detected.
Contribution
It introduces new operational capabilities of Swift enabling follow-up within 15-20 minutes, significantly reducing latency in high-energy transient observations.
Findings
No coincident emission detected at T0 or T0+32 minutes.
Swift operational capabilities allow follow-up within 15-20 minutes.
Demonstrated the technical feasibility of ultra-low latency high-energy follow-up.
Abstract
We report results of a novel high-energy follow-up observation of a potential Fast Radio Burst. The radio burst was detected by VLA/realfast and followed-up by the Neil Gehrels Swift Observatory in very low latency utilizing new operational capabilities of Swift (arXiv:2005.01751), with pointed soft X-ray and UV observations beginning at T0+32 minutes, and hard X-ray/gamma-ray event data saved around T0. These observations are x faster than previous X-ray/UV follow-up of any radio transient to date. No emission is seen coincident with the FRB candidate at T0, with a 0.2s fluence upper limit of erg cm (14-195 keV) for a SGR 1935+2154-like flare, nor at T0+32 minutes down to upper limits of 22.18 AB mag in UVOT u band, and erg cm s from 0.3-10 keV for the 2 ks observation. The candidate FRB alone is not…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Pulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations
