A Decade and a Half of Fast Radio Burst Observations

Fast radio bursts (FRBs) have a story which has been told and retold many times over the past few years as they have sparked excitement and controversy since their pioneering discovery in 2007. The FRB class encompasses a number of microsecond- to millisecond-duration pulses occurring at Galactic to cosmological distances with energies spanning about 8 orders of magnitude. While most FRBs have been observed as singular events, a small fraction of them have been observed to repeat over various timescales leading to an apparent dichotomy in the population. & SIM;50 unique progenitor theories have been proposed, but no consensus has emerged for their origin(s). However, with the discovery of an FRB-like pulse from the Galactic magnetar SGR J1935+2154, magnetar engine models are the current leading theory. Overall, FRB pulses exhibit unique characteristics allowing us to probe line-of-sight magnetic field strengths, inhomogeneities in the intergalactic/interstellar media, and plasma turbulence through an assortment of extragalactic and cosmological propagation effects. Consequently, they are formidable tools to study the Universe. This review follows the progress of the field between 2007 and 2020 and presents the science highlights of the radio observations.

Automated summary

Fast radio bursts (FRBs) have been a subject of excitement and controversy since their discovery in 2007, with various theories proposed for their origin. Recent observations of FRB-like pulses from Galactic magnetars have led to magnetar engine models emerging as the leading theory in understanding these mysterious phenomena. Overall, FRB pulses offer unique characteristics for probing magnetic field strengths, interstellar media inhomogeneities, and plasma turbulence, making them important tools for studying the Universe.