activity
20152021
most citedThe Phase II Murchison Widefield Array: Design Overview

240 citations · 950 across the 21 of their papers we have counts for

collaborators

21 papers

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★ 2 cited

The Aperture Array Verification System 1: System overview and early commissioning results

P. Benthem, R. Wayth, E. de Lera Acedo +51

The design and development process for the Square Kilometre Array (SKA) radio telescope, the Low Frequency Aperture Array component, was progressed during the SKA pre-construction…

astro-ph.IM2021★ 16 cited

Dual Polarization Measurements of MWA Beampatterns at 137 MHz

A. Chokshi, J. L. B. Line, N. Barry +5

The wide adoption of low-frequency radio interferometers as a tool for deeper and higher resolution astronomical observations has revolutionised radio astronomy. Despite their cons…

astro-ph.IM2020★ 4 cited

The SKA Particle Array Prototype: The First Particle Detector at the Murchison Radio-astronomy Observatory

J. D. Bray, A. Williamson, J. Schelfhout +18

We report on the design, deployment, and first results from a scintillation detector deployed at the Murchison Radio-astronomy Observatory (MRO). The detector is a prototype for a…

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…