The path to the low frequency Square Kilometre Array in Australia

The Square Kilometre Array (SKA) is a planned next-generation radio telescope to be constructed at two locations, in Western Australia and Southern Africa, utilising a range of antenna technologies to cover the radio frequency range required to satisfy its science goals. The SKA pushes the boundarie...

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Main Authors: Tingay, Steven, Hall, Peter
Format: Journal Article
Published: 2012
Online Access:http://astronomy.curtin.edu.au/local/docs/SKA.pdf
http://hdl.handle.net/20.500.11937/34481
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author Tingay, Steven
Hall, Peter
author_facet Tingay, Steven
Hall, Peter
author_sort Tingay, Steven
building Curtin Institutional Repository
collection Online Access
description The Square Kilometre Array (SKA) is a planned next-generation radio telescope to be constructed at two locations, in Western Australia and Southern Africa, utilising a range of antenna technologies to cover the radio frequency range required to satisfy its science goals. The SKA pushes the boundaries of physics and engineering on a number of fronts simultaneously and is thus a very ambitious project with innovation at its heart. In this article we consider the component of the SKA to be built in Western Australia in full scope, a survey telescope designed for very early Universe cosmology, operating at low radio frequencies. The path to the low frequency SKA in Australia involves precursor instrumentation, SKA pre-construction activities, and the deployment of the final instrument in two phases over approximately the next decade.
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spelling curtin-20.500.11937-344812017-01-30T13:43:45Z The path to the low frequency Square Kilometre Array in Australia Tingay, Steven Hall, Peter The Square Kilometre Array (SKA) is a planned next-generation radio telescope to be constructed at two locations, in Western Australia and Southern Africa, utilising a range of antenna technologies to cover the radio frequency range required to satisfy its science goals. The SKA pushes the boundaries of physics and engineering on a number of fronts simultaneously and is thus a very ambitious project with innovation at its heart. In this article we consider the component of the SKA to be built in Western Australia in full scope, a survey telescope designed for very early Universe cosmology, operating at low radio frequencies. The path to the low frequency SKA in Australia involves precursor instrumentation, SKA pre-construction activities, and the deployment of the final instrument in two phases over approximately the next decade. 2012 Journal Article http://hdl.handle.net/20.500.11937/34481 http://astronomy.curtin.edu.au/local/docs/SKA.pdf restricted
spellingShingle Tingay, Steven
Hall, Peter
The path to the low frequency Square Kilometre Array in Australia
title The path to the low frequency Square Kilometre Array in Australia
title_full The path to the low frequency Square Kilometre Array in Australia
title_fullStr The path to the low frequency Square Kilometre Array in Australia
title_full_unstemmed The path to the low frequency Square Kilometre Array in Australia
title_short The path to the low frequency Square Kilometre Array in Australia
title_sort path to the low frequency square kilometre array in australia
url http://astronomy.curtin.edu.au/local/docs/SKA.pdf
http://hdl.handle.net/20.500.11937/34481