collaborators

10 papers

astro-ph.HE2026

Two new highly scattered fast radio bursts: evidence for scatter broadening by the circumsource medium

Joscha N. Jahns-Schindler, Keith W. Bannister, Adam T. Deller +17

We found two highly scattered Fast Radio Bursts (FRBs) during commissioning of the Commensal Realtime ASKAP Fast Transient COherent (CRACO) backend. FRB 240210D and FRB 240312D hav…

astro-ph.IM2026

VASTER: The ASKAP real-time fast-imaging pipeline -- overview and discovery of two long period transients

Yuanming Wang, Dougal Dobie, Tara Murphy +22

Recent developments in widefield radio telescopes have enabled searches of a new region of parameter space in the time domain: timescales of seconds to minutes, that have been over…

astro-ph.CO2026

Modelling DSA, FAST and CRAFT surveys in a z-DM analysis and constraining a minimum FRB energy

Jordan Hoffmann, Clancy W. James, Marcin Glowacki +5

Fast radio burst (FRB) science primarily revolves around two facets: the origin of these bursts and their use in cosmological studies. This work follows from previous redshift-disp…

astro-ph.HE2026

A fast radio burst cyclone in technicolour: evidence of plasma lensing

Pavan A. Uttarkar, Ryan M. Shannon, Kelly Gourdji +9

Fast radio bursts (FRBs) are bright, energetic, radio pulses of extragalactic origin. A dichotomy has emerged in the population: some produce repeat bursts, while the majority do n…

astro-ph.GA2025

Mapping the Spatial Distribution of Fast Radio Bursts within their Host Galaxies

Alexa C. Gordon, Wen-fai Fong, Adam T. Deller +23

We present deep optical and near-infrared observations of the host galaxies of 34 fast radio bursts (FRBs) detected by the Commensal Real-time ASKAP Fast Transient (CRAFT) survey o…

astro-ph.HE2025

The discovery of a 41s radio pulsar PSR J0311+1402 with ASKAP

Yuanming Wang, Pavan Uttarkar, Ryan Shannon +16

The emerging population of long-period radio transients (LPTs) show both similarities and differences with normal pulsars. A key difference is that their radio emission is too brig…