activity
20172019
most citedFollow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

212 citations · 424 across the 7 of their papers we have counts for

collaborators

15 papers

astro-ph.CO201998 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.IM201935 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.IM201910 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

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…

astro-ph.CO201932 cited

Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array

Cathryn M. Trott, Catherine A. Watkinson, Christopher H. Jordan +42

We apply two methods to estimate the 21~cm bispectrum from data taken within the Epoch of Reionisation (EoR) project of the Murchison Widefield Array (MWA). Using data acquired wit…

astro-ph.HE201816 cited

Hunting for radio emission from the intermittent pulsar J1107-5907 at low frequencies

B. W. Meyers, S. E. Tremblay, N. D. R. Bhat +30

The rare intermittent pulsars pose some of the most challenging questions surrounding the pulsar emission mechanism, but typically have relatively minimal low-frequency (