activity
20092021
most citedThe Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

1.3k citations · 5.9k across the 52 of their papers we have counts for

collaborators

53 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

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.IM2016★ 170 cited

First Season MWA EoR Power Spectrum Results at Redshift 7

A. P. Beardsley, B. J. Hazelton, I. S. Sullivan +63

The Murchison Widefield Array (MWA) has collected hundreds of hours of Epoch of Reionization (EoR) data and now faces the challenge of overcoming foreground and systematic contamin…

astro-ph.GA2016★ 80 cited

Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic pole

Emil Lenc, B. M. Gaensler, X. H. Sun +76

We present deep polarimetric observations at 154 MHz with the Murchison Widefield Array (MWA), covering 625 deg^2 centered on RA=0 h, Dec=-27 deg. The sensitivity available in our…

astro-ph.IM2016★ 34 cited

A High Reliability Survey of Discrete Epoch of Reionization Foreground Sources in the MWA EoR0 Field

P. A. Carroll, J. Line, M. F. Morales +61

Detection of the Epoch of Reionization HI signal requires a precise understanding of the intervening galaxies and AGN, both for instrumental calibration and foreground removal. We…