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  5. Limits on Fast Radio Bursts and other transient sources at 182 MHz using the Murchison Widefield Array
 

Limits on Fast Radio Bursts and other transient sources at 182 MHz using the Murchison Widefield Array

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2016
Author(s)
Rowlinson, A.
•
Bell, M. E.
•
Murphy, T.
•
Trott, C. M.
•
Hurley-Walker, N.
•
Johnston, S.
•
Tingay, S. J.
•
Kaplan, D. L.
•
Carbone, D.
•
Hancock, P. J.
•
Feng, L.
•
Offringa, A. R.
•
BERNARDI, GIANNI  
•
Bowman, J. D.
•
Briggs, F.
•
Cappallo, R. J.
•
Deshpande, A. A.
•
Gaensler, B. M.
•
Greenhill, L. J.
•
Hazelton, B. J.
•
Johnston-Hollitt, M.
•
Lonsdale, C. J.
•
McWhirter, S. R.
•
Mitchell, D. A.
•
Morales, M. F.
•
Morgan, E.
•
Oberoi, D.
•
Ord, S. M.
•
Prabu, T.
•
Udaya Shankar, N.
•
Srivani, K. S.
•
Subrahmanyan, R.
•
Wayth, R. B.
•
Webster, R. L.
•
Williams, A.
•
Williams, C. L.
DOI
10.1093/mnras/stw451
Abstract
We present a survey for transient and variable sources, on time-scales from 28 s to ∼1 yr, using the Murchison Widefield Array (MWA) at 182 MHz. Down to a detection threshold of 0.285 Jy, no transient candidates were identified, making this the most constraining low-frequency survey to date and placing a limit on the surface density of transients of <4.1 × 10-7 deg-2 for the shortest time-scale considered. At these frequencies, emission from Fast Radio Bursts (FRBs) is expected to be detectable in the shortest time-scale images without any corrections for interstellar or intergalactic dispersion. At an FRB limiting flux density of 7980 Jy, we find a rate of <82 FRBs per sky per day for dispersion measures <700 pc cm-3. Assuming a cosmological population of standard candles, our rate limits are consistent with the FRB rates obtained by Thornton et al. if they have a flat spectral slope. Finally, we conduct an initial variability survey of sources in the field with flux densities ≳0.5 Jy and identify no sources with significant variability in their light curves. However, we note that substantial further work is required to fully characterize both the short-term and low-level variability within this field.
Volume
458
Issue
4
Start page
3506
Uri
http://hdl.handle.net/20.500.12386/26337
Url
https://academic.oup.com/mnras/article/458/4/3506/2613802
Issn Identifier
0035-8711
Ads BibCode
2016MNRAS.458.3506R
Rights
open.access
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