activity
20122017
most citedThe Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

1.3k citations · 1.7k across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2017★ 21 cited

The Engineering Development Array: A low frequency radio telescope utilising SKA precursor technology

Randall Wayth, Marcin Sokolowski, Tom Booler +21

We describe the design and performance of the Engineering Development Array (EDA), which is a low frequency radio telescope comprising 256 dual-polarisation dipole antennas working…

astro-ph.IM2017★ 2 cited

Revisiting Hybrid Interferometry with Low-Frequency Radio Astronomy Arrays

Adrian T. Sutinjo, Daniel Ung, Tim M. Colegate +3

Radio interferometry most commonly involves antennas or antenna arrays of identical design. The identical antenna assumption leads to a convenient and useful mathematical simplific…

astro-ph.HE2017★ 165 cited

The detection of an extremely bright fast radio burst in a phased array feed survey

Keith Bannister, Ryan Shannon, Jean-Pierre Macquart +53

We report the detection of an ultra-bright fast radio burst (FRB) from a modest, 3.4-day pilot survey with the Australian Square Kilometre Array Pathfinder. The survey was conducte…

astro-ph.IM2015★ 72 cited

Characterization of a Low-Frequency Radio Astronomy Prototype Array in Western Australia

A. T. Sutinjo, T. M. Colegate, R. B. Wayth +12

We report characterization results for an engineering prototype of a next-generation low-frequency radio astronomy array. This prototype, which we refer to as the Aperture Array Ve…

astro-ph.IM2015★ 4 cited

Antenna array characterization via radio interferometry observation of astronomical sources

T. M. Colegate, A. T. Sutinjo, P. J. Hall +12

We present an in-situ antenna characterization method and results for a "low-frequency" radio astronomy engineering prototype array, characterized over the 75-300 MHz frequency ran…

astro-ph.IM2015★ 137 cited

BIGHORNS - Broadband Instrument for Global HydrOgen ReioNisation Signal

M. Sokolowski, S. E. Tremblay, R. B. Wayth +12

The redshifted 21cm line of neutral hydrogen (HI), potentially observable at low radio frequencies (~50-200 MHz), should be a powerful probe of the physical conditions of the inter…