activity
20082021
most citedWSClean: an implementation of a fast, generic wide-field imager for radio astronomy

937 citations · 4.4k across the 55 of their papers we have counts for

collaborators

55 papers

astro-ph.GA2021★ 7 cited

The GLEAM 200 MHz Local Radio Luminosity Function for AGN and Star-forming Galaxies

T. M. O. Franzen, N. Seymour, E. M. Sadler +24

The GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) is a radio continuum survey at 76-227 MHz of the entire southern sky (Declination ) with an angular…

astro-ph.GA2020★ 12 cited

Searching for Dark Matter Signals from Local Dwarf Spheroidal Galaxies at Low Radio Frequencies in the GLEAM Survey

Robin H. W. Cook, Nick Seymour, Kristine Spekkens +18

The search for emission from weakly interacting massive particle (WIMP) dark matter annihilation and decay has become a multi-pronged area of research not only targeting a diverse…

astro-ph.GA2019★ 60 cited

GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane ,

Natasha Hurley-Walker, Paul J. Hancock, Thomas M. O. Franzen +16

This work makes available a further 2,860deg of the GLEAM survey, covering half of the accessible Galactic Plane, across twenty frequency bands sampling MHz, with resol…

astro-ph.HE2019★ 27 cited

New candidate radio supernova remnants detected in the GLEAM survey over ,

Natasha Hurley-Walker, Miroslav D. Filipovic, Bryan M. Gaensler +18

We have detected 27 new supernova remnants (SNRs) using a new data release of the GLEAM survey from the Murchison Widefield Array (MWA) telescope, including the lowest surface-brig…

astro-ph.HE2019★ 35 cited

Candidate radio supernova remnants observed by the GLEAM survey over and

Natasha Hurley-Walker, Bryan M. Gaensler, Denis A. Leahy +18

We examined the latest data release from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey covering , $180^\circ < l < 240^\…

astro-ph.SR2019★ 12 cited

A Radio Census of the Massive Stellar Cluster Westerlund 1

H. Andrews, D. Fenech, R. K. Prinja +2

Massive stars and their stellar winds are important for a number of feedback processes. The mass lost in the stellar wind can help determine the end-point of the star as a NS or a…