activity
20042022
most citedFollow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

212 citations · 932 across the 31 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.IM2021★ 1 cited

The Engineering Development Array 2: design, performance and lessons from an SKA-Low prototype station

Randall Wayth, Marcin Sokolowski, Jess Broderick +21

We present the Engineering Development Array 2, which is one of two instruments built as a second generation prototype station for the future Square Kilometre Array Low Frequency A…

astro-ph.IM2021

Characterization of the SKA1-Low prototype station Aperture Array Verification System 2

Giulia Macario, Giuseppe Pupillo, Gianni Bernardi +16

The low frequency component of the Square Kilometre Array (SKA1-Low) will be an aperture phased array located at the Murchison Radio-astronomy Observatory (MRO) site in Western Aus…

astro-ph.HE2021★ 17 cited

Murchison Widefield Array rapid-response observations of the short GRB 180805A

G. E. Anderson, P. J. Hancock, A. Rowlinson +14

Here we present stringent low-frequency 185MHz limits on coherent radio emission associated with a short gamma-ray burst (SGRB). Our observations of the short GRB 180805A were take…

astro-ph.HE2021★ 19 cited

Discovery of a steep-spectrum low-luminosity pulsar with the Murchison Widefield Array

N. A. Swainston, N. D. R. Bhat, M. Sokolowski +17

We report the discovery of the first new pulsar with the Murchison Widefield Array (MWA), PSR J00361033, a long-period (0.9 s) nonrecycled pulsar with a dispersion measure (DM)…

astro-ph.IM2021★ 16 cited

A Southern-Hemisphere all-sky radio transient monitor for SKA-Low prototype stations

M. Sokolowski, R. B. Wayth, N. D. R. Bhat +20

We present the first southern-hemisphere all-sky imager and radio-transient monitoring system implemented on two prototype stations of the low-frequency component of the Square Kil…

astro-ph.IM2021

Imaging at 300 MHz With the MWA

J. H. Cook, N. Seymour, M. Sokolowski

At relatively high frequencies, highly sensitive grating sidelobes occur in the primary beam patterns of low frequency aperture arrays (LFAA) such as the Murchison Widefield Array…