activity
20122015
most citedBIGHORNS - Broadband Instrument for Global HydrOgen ReioNisation Signal

137 citations · 314 across the 6 of their papers we have counts for

collaborators

6 papers

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★ 26 cited

The impact of the ionosphere on ground-based detection of the global Epoch of Reionisation signal

Marcin Sokolowski, Randall B. Wayth, Steven E. Tremblay +7

The redshifted 21cm line of neutral hydrogen (Hi), potentially observable at low radio frequencies (~50-200 MHz), is a promising probe of the physical conditions of the inter-galac…

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…

astro-ph.IM2014★ 74 cited

Understanding Instrumental Stokes Leakage in Murchison Widefield Array Polarimetry

Adrian Sutinjo, John O'Sullivan, Emil Lenc +4

This paper offers an electromagnetic, more specifically array theory, perspective on understanding strong instrumental polarization effects for planar low-frequency "aperture array…

astro-ph.IM2012★ 1 cited

Square Kilometre Array station configuration using two-stage beamforming

Aziz Jiwani, Tim Colegate, Nima Razavi-Ghods +3

The lowest frequency band (70 - 450 MHz) of the Square Kilometre Array will consist of sparse aperture arrays grouped into geographically-localised patches, or stations. Signals fr…