We summarize our understanding of millisecond radio bursts from an extragalactic
population of sources. Fast radio bursts (FRBs) occur at an extraordinary rate, thousands per …

At present, we have almost as many theories to explain Fast Radio Bursts as we have Fast
Radio Bursts observed. This landscape will be changing rapidly with CHIME/FRB, recently …

We present observations and detailed characterizations of five new host galaxies of fast
radio bursts (FRBs) discovered with the Australian Square Kilometre Array Pathfinder …

The polarization of fast radio bursts (FRBs), which are bright astronomical transient
phenomena, contains information about their environments. Using wide-band observations …

Fast radio bursts (FRBs) can arise from synchrotron maser emission at ultrarelativistic
magnetized shocks, such as produced by flare ejecta from young magnetars. We combine …

The discovery of radio pulsars over a half century ago was a seminal moment in astronomy.
It demonstrated the existence of neutron stars, gave a powerful observational tool to study …

Fast radio bursts (FRBs) are millisecond-duration radio transients, of unknown origin. Two
possible mechanisms that could generate extremely coherent emission from FRBs invoke …

We constrain the Hubble constant H 0 using Fast Radio Burst (FRB) observations from the
Australian Square Kilometre Array Pathfinder (ASKAP) and Murriyang (Parkes) radio …

Combining high time and frequency resolution full-polarization spectra of fast radio bursts
(FRBs) with knowledge of their host galaxy properties provides an opportunity to study both …

We report the discovery of four Fast Radio Bursts (FRBs) in the ongoing SUrvey for Pulsars
and Extragalactic Radio Bursts at the Parkes Radio Telescope: FRBs 150610, 151206 …