Searching for Fast Radio Transients with SKA Phase 1

The Square Kilometre Array (SKA) provides an excellent opportunity for low-cost searches for fast radio transients. The increased sensitivity and field of view of the SKA compared with other radio telescopes will make it an ideal instrument to search for impulsive emission from high–energy density e...

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Main Authors: Colegate, Timothy, Clarke, Nathan
Format: Journal Article
Published: CSIRO 2011
Online Access:http://hdl.handle.net/20.500.11937/3955
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author Colegate, Timothy
Clarke, Nathan
author_facet Colegate, Timothy
Clarke, Nathan
author_sort Colegate, Timothy
building Curtin Institutional Repository
collection Online Access
description The Square Kilometre Array (SKA) provides an excellent opportunity for low-cost searches for fast radio transients. The increased sensitivity and field of view of the SKA compared with other radio telescopes will make it an ideal instrument to search for impulsive emission from high–energy density events. We present a high-level search ‘use case’ and propose “event rate per unit cost” as a figure of merit to compare transient survey strategies for radio telescope arrays; we use “event rate per beam formed and searched” as a first-order approximation of this measure. Key results are that incoherent (phase-insensitive) combination of antenna signals achieves the highest event rate per beam, and that 50–100 MHz processed bandwidth is sufficient for extragalactic searches with SKA Phase 1; the gain in event rate from using the full available bandwidth is small. Greater system flexibility will enable more effective searches, but need not drive the top-level system requirements beyond those already proposed for the SKA. The most appropriate search strategy depends on the observed sky direction and the source population; for SKA Phase 1, low-frequency aperture arrays tend to be more effective for extragalactic searches, and dishes more effective for directions of increased scatter broadening, such as near the Galactic plane.
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spelling curtin-20.500.11937-39552017-09-13T16:07:59Z Searching for Fast Radio Transients with SKA Phase 1 Colegate, Timothy Clarke, Nathan The Square Kilometre Array (SKA) provides an excellent opportunity for low-cost searches for fast radio transients. The increased sensitivity and field of view of the SKA compared with other radio telescopes will make it an ideal instrument to search for impulsive emission from high–energy density events. We present a high-level search ‘use case’ and propose “event rate per unit cost” as a figure of merit to compare transient survey strategies for radio telescope arrays; we use “event rate per beam formed and searched” as a first-order approximation of this measure. Key results are that incoherent (phase-insensitive) combination of antenna signals achieves the highest event rate per beam, and that 50–100 MHz processed bandwidth is sufficient for extragalactic searches with SKA Phase 1; the gain in event rate from using the full available bandwidth is small. Greater system flexibility will enable more effective searches, but need not drive the top-level system requirements beyond those already proposed for the SKA. The most appropriate search strategy depends on the observed sky direction and the source population; for SKA Phase 1, low-frequency aperture arrays tend to be more effective for extragalactic searches, and dishes more effective for directions of increased scatter broadening, such as near the Galactic plane. 2011 Journal Article http://hdl.handle.net/20.500.11937/3955 10.1071/AS11031 CSIRO unknown
spellingShingle Colegate, Timothy
Clarke, Nathan
Searching for Fast Radio Transients with SKA Phase 1
title Searching for Fast Radio Transients with SKA Phase 1
title_full Searching for Fast Radio Transients with SKA Phase 1
title_fullStr Searching for Fast Radio Transients with SKA Phase 1
title_full_unstemmed Searching for Fast Radio Transients with SKA Phase 1
title_short Searching for Fast Radio Transients with SKA Phase 1
title_sort searching for fast radio transients with ska phase 1
url http://hdl.handle.net/20.500.11937/3955