activity
20132026
most citedA measurement of Hubble's Constant using Fast Radio Bursts

124 citations · 986 across the 44 of their papers we have counts for

collaborators

47 papers

astro-ph.GA2026

A Relationship Between Fast Radio Burst Dispersion Measure and Host Galaxy Inclination

Lachlan Marnoch, Stuart D. Ryder, Sunil Simha +9

It is commonly thought that fast radio bursts (FRBs) trace star formation, and that they are produced by magnetars. Both hypotheses imply that their sources are hosted primarily (b…

astro-ph.CO2026

Bayesian Galaxy Asymmetry

Mathieu Perron-Cormier, Kristine Spekkens, Nathan Deg +2

Galaxy asymmetry is an efficient way to characterize galaxy morphology in atomic hydrogen 21 cm emission detections. We propose a novel Bayesian approach to calculate the probabili…

astro-ph.HE2026

CRAFT HTR2: Polarimetry of 64 non-repeating fast radio bursts from the updated CRAFT catalogue

T. Dial, A. T. Deller, Marcin Glowacki +6

We present high-time resolution spectro-polarimetric data for 34 new fast radio bursts (FRBs) discovered by the Commensal Real-time Fast Transients (CRAFT) survey on the Australian…

astro-ph.IM2026

Enhanced Astrometry of the Rapid ASKAP Continuum Survey: Mid and High Frequency Epochs

Akhil Jaini, Adam T. Deller, Yuanming Wang +4

Accurate radio astrometry is essential for reliable cross-identification of sources across wavelengths, precision localisation of transient events, and the construction of stable a…

astro-ph.GA2026

MIGHTEE-HI: HI catalogue of 293 sources for the COSMOS field and comparative study of 3-dimensional source finding methods

Michalina Maksymowicz-Maciata, Natasha Maddox, Catherine Hale +12

We present a catalogue of HI sources extracted from the MIGHTEE survey data cubes covering the COSMOS field. The catalogue contains 293 sources in the redshift range of 0.004 < z <…

astro-ph.IM2026

A PINK update: Improvements to the CELEBI fast radio burst data reduction and analysis pipeline

M. Glowacki, T. Dial, A. Bera +9

Fast radio bursts (FRBs) which are well localised (1") to their host galaxy are tools for studying cosmology and the intergalactic medium. Furthermore, high-time resolution data…