activity
20122021
most citedThe Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

1.3k citations · 2.4k across the 23 of their papers we have counts for

collaborators

24 papers

astro-ph.IM2021★ 145 cited

SoFiA 2 -- An automated, parallel HI source finding pipeline for the WALLABY survey

T. Westmeier, S. Kitaeff, D. Pallot +12

We present SoFiA 2, the fully automated 3D source finding pipeline for the WALLABY extragalactic HI survey with the Australian SKA Pathfinder (ASKAP). SoFiA 2 is a reimplementation…

astro-ph.IM2020★ 9 cited

Calibration database for the Murchison Widefield Array All-Sky Virtual Observatory

M. Sokolowski, C. H. Jordan, G. Sleap +11

We present a calibration component for the Murchison Widefield Array All-Sky Virtual Observatory (MWA ASVO) utilising a newly developed PostgreSQL database of calibration solutions…

astro-ph.CO2019★ 98 cited

First Season MWA Phase II EoR Power Spectrum Results at Redshift 7

W. Li, J. C. Pober, N. Barry +44

The compact configuration of Phase II of the Murchison Widefield Array (MWA) consists of both a redundant subarray and pseudo-random baselines, offering unique opportunities to per…

astro-ph.IM2019★ 35 cited

Science with the Murchison Widefield Array: Phase I Results and Phase II Opportunities

A. P. Beardsley, M. Johnston-Hollitt, C. M. Trott +56

The Murchison Widefield Array (MWA) is an open access telescope dedicated to studying the low frequency (80300 MHz) southern sky. Since beginning operations in mid 2013, the MWA…

astro-ph.IM2019★ 10 cited

A VOEvent based automatic trigger system for the Murchison Widefield Array

P. J. Hancock, G. E. Anderson, A. Williams +22

The Murchison Widefield Array (MWA) is an electronically steered low frequency (\,MHz) radio interferometer, with a `slew' time less than 8seconds. Low frequency (\…

astro-ph.HE2019★ 10 cited

A high time resolution study of the millisecond pulsar J2241-5236 at frequencies below 300 MHz

D. Kaur, N. D. R. Bhat, S. E. Tremblay +20

One of the major challenges for pulsar timing array (PTA) experiments is the mitigation of the effects of the turbulent interstellar medium (ISM) from timing data. These can potent…