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The High Time and Frequency Resolution Capabilities of the Murchison Widefield Array

Authors :
Tremblay, S. E.
Ord, S. M.
Bhat, N. D. R.
Tingay, S. J.
Crosse, B.
Pallot, D.
Oronsaye, S. I.
Bernardi, G.
Bowman, J. D.
Briggs, F.
Cappallo, R. J.
Corey, B. E.
Deshpande, A. A.
Emrich, D.
Goeke, R.
Greenhill, L. J.
Hazelton, B. J.
Johnston-Hollitt, M.
Kaplan, D. L.
Kasper, J. C.
Kratzenberg, E.
Lonsdale, C. J.
Lynch, M. J.
McWhirter, S. R.
Mitchell, D. A.
Morales, M. F.
Morgan, E.
Oberoi, D.
Prabu, T.
Rogers, A. E. E.
Roshi, A.
Shankar, N. Udaya
Srivani, K. S.
Subrahmanyan, R.
Waterson, M.
Wayth, R. B.
Webster, R. L.
Whitney, A. R.
Williams, A.
Williams, C. L.
Publication Year :
2015

Abstract

The science cases for incorporating high time resolution capabilities into modern radio telescopes are as numerous as they are compelling. Science targets range from exotic sources such as pulsars, to our Sun, to recently detected possible extragalactic bursts of radio emission, the so-called fast radio bursts (FRBs). Originally conceived purely as an imaging telescope, the initial design of the Murchison Widefield Array (MWA) did not include the ability to access high time and frequency resolution voltage data. However, the flexibility of the MWA's software correlator allowed an off-the-shelf solution for adding this capability. This paper describes the system that records the 100 micro-second and 10 kHz resolution voltage data from the MWA. Example science applications, where this capability is critical, are presented, as well as accompanying commissioning results from this mode to demonstrate verification.<br />Comment: 9 pages, 6 figures, 1 table. Accepted for publication in PASA

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1501.05723
Document Type :
Working Paper
Full Text :
https://doi.org/10.1017/pasa.2015.6