activity
20152023
most citedA repeating fast radio burst source localised to a nearby spiral galaxy

436 citations · 824 across the 16 of their papers we have counts for

collaborators

23 papers

astro-ph.IM202227 cited

CASA on the fringe -- Development of VLBI processing capabilities for CASA

Ilse M. van Bemmel, Mark Kettenis, Des Small +14

New functionality to process Very Long Baseline Interferometry (VLBI) data has been implemented in the CASA package. This includes two new tasks to handle fringe fitting and VLBI-s…

astro-ph.SR202210 cited

Optical and NIR data and modelling of nova V5668 Sgr

L. Takeda, M. Diaz, R. D. Campbell +4

We present HST optical images, Keck-OSIRIS NIR IFS data cubes and Keck-NIRC2 NIR images of nova V5668 Sgr from 2016 to 2019. The observations indicate enhanced emission at the pola…

astro-ph.IM2021

Robust Assessment of Clustering Methods for Fast Radio Transient Candidates

Kshitij Aggarwal, Sarah Burke-Spolaor, Casey J. Law +7

Fast radio transient search algorithms identify signals of interest by iterating and applying a threshold on a set of matched filters. These filters are defined by properties of th…

astro-ph.HE2021

Probing the reach of the Intermediate Polar Cataclysmic Variable Population with Swift J183920.1-045350

Nicholas M. Gorgone, Patrick A. Woudt, David Buckley +18

We report on the Swift/XRT Deep Galactic Plane Survey discovery and multi-wavelength follow-up observations of a new intermediate polar Cataclysmic Variable, Swift J183920.1-045350…

astro-ph.HE2021

Constraints on the Sub-pc Environment of the Nearby Type Iax SN 2014dt from Deep X-ray and Radio Observations

Candice M. Stauffer, Raffaella Margutti, Justin D. Linford +8

We present X-ray and radio observations of what may be the closest type Iax supernova (SN) to date, SN 2014dt (d=12.3-19.3 Mpc) and provide tight constraints on the radio and X-ray…

astro-ph.HE202174 cited

Rapid Spectral Variability of a Giant Flare from a Magnetar in NGC 253

O. J. Roberts, P. Veres, M. G. Baring +18

Magnetars are slowly-rotating neutron stars with extremely strong magnetic fields ( G), episodically emitting ms long X-ray bursts with energies of $\sim10^{4…