W. Arcus
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View article: The fast radio burst population energy distribution
The fast radio burst population energy distribution Open
We examine the energy distribution of the fast radio burst (FRB) population using a well-defined sample of 63 FRBs from the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope, 28 of which are localised to a host galaxy. W…
View article: The Fast Radio Burst Population Energy Distribution
The Fast Radio Burst Population Energy Distribution Open
We examine the energy distribution of the fast radio burst (FRB) population using a well-defined sample of 63 FRBs from the ASKAP radio telescope, 28 of which are localised to a host galaxy. We apply the luminosity-volume ($V/V_{\mathrm{ma…
View article: Comparison of the Parkes and FAST FRB DM distribution
Comparison of the Parkes and FAST FRB DM distribution Open
We model the fast radio burst (FRB) dispersion measure (DM) distribution for the Five-hundred-meter Aperture Spherical Telescope (FAST) and compare this with the four FRBs published in the literature to date. We compare the DM distribution…
View article: The fast radio burst dispersion measure distribution
The fast radio burst dispersion measure distribution Open
We compare the dispersion measure (DM) statistics of FRBs detected by the ASKAP and Parkes radio telescopes. We jointly model their DM distributions, exploiting the fact that the telescopes have different survey fluence limits but likely s…
View article: A single fast radio burst localized to a massive galaxy at cosmological distance
A single fast radio burst localized to a massive galaxy at cosmological distance Open
Pinpointing a single fast radio burst Fast radio bursts (FRBs) are flashes of radio emission from distant astronomical sources. Two FRBs are known to have repeated, but most last just a few milliseconds and are never seen again. Most teles…