High time resolution radio astronomy with low-frequency interferometric arrays

High time resolution applications of radio astronomy including pulsars and fast radio bursts are proving to be incredibly scientifically rewarding in terms of the depth and breadth of new physics and astrophysics they unveil. While the use of large single-dish type instruments has been dominating th...

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Main Authors: Bhat, N., Ord, Stephen, Tremblay, S., Tingay, Steven, Deshpande, A., Van Straten, W.
Format: Conference Paper
Published: Institute of Electrical and Electronics Engineers Inc. 2014
Online Access:http://hdl.handle.net/20.500.11937/30893
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author Bhat, N.
Ord, Stephen
Tremblay, S.
Tingay, Steven
Deshpande, A.
Van Straten, W.
author_facet Bhat, N.
Ord, Stephen
Tremblay, S.
Tingay, Steven
Deshpande, A.
Van Straten, W.
author_sort Bhat, N.
building Curtin Institutional Repository
collection Online Access
description High time resolution applications of radio astronomy including pulsars and fast radio bursts are proving to be incredibly scientifically rewarding in terms of the depth and breadth of new physics and astrophysics they unveil. While the use of large single-dish type instruments has been dominating the field over the past decades, with the emergence of several next-generation radio facilities including the Square Kilometre Array (SKA) pre-cursors and pathfinders, it becomes imperative to develop and master suitable high time resolution functionalities that are effective for interferometric instruments. The Murchison Widefield Array (MWA) - the low-frequency pre-cursor to the SKA - provides excellent opportunities to help realise the related goals. This paper will describe the high time resolution mode being developed for the MWA and highlight early science results, including the lowest-frequency scintillation observations of the millisecond pulsar PSR J0437-4715.
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institution Curtin University Malaysia
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publishDate 2014
publisher Institute of Electrical and Electronics Engineers Inc.
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spelling curtin-20.500.11937-308932017-09-13T15:12:58Z High time resolution radio astronomy with low-frequency interferometric arrays Bhat, N. Ord, Stephen Tremblay, S. Tingay, Steven Deshpande, A. Van Straten, W. High time resolution applications of radio astronomy including pulsars and fast radio bursts are proving to be incredibly scientifically rewarding in terms of the depth and breadth of new physics and astrophysics they unveil. While the use of large single-dish type instruments has been dominating the field over the past decades, with the emergence of several next-generation radio facilities including the Square Kilometre Array (SKA) pre-cursors and pathfinders, it becomes imperative to develop and master suitable high time resolution functionalities that are effective for interferometric instruments. The Murchison Widefield Array (MWA) - the low-frequency pre-cursor to the SKA - provides excellent opportunities to help realise the related goals. This paper will describe the high time resolution mode being developed for the MWA and highlight early science results, including the lowest-frequency scintillation observations of the millisecond pulsar PSR J0437-4715. 2014 Conference Paper http://hdl.handle.net/20.500.11937/30893 10.1109/URSIGASS.2014.6930047 Institute of Electrical and Electronics Engineers Inc. restricted
spellingShingle Bhat, N.
Ord, Stephen
Tremblay, S.
Tingay, Steven
Deshpande, A.
Van Straten, W.
High time resolution radio astronomy with low-frequency interferometric arrays
title High time resolution radio astronomy with low-frequency interferometric arrays
title_full High time resolution radio astronomy with low-frequency interferometric arrays
title_fullStr High time resolution radio astronomy with low-frequency interferometric arrays
title_full_unstemmed High time resolution radio astronomy with low-frequency interferometric arrays
title_short High time resolution radio astronomy with low-frequency interferometric arrays
title_sort high time resolution radio astronomy with low-frequency interferometric arrays
url http://hdl.handle.net/20.500.11937/30893