The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigation
A. R. Offringa, R. B. Wayth, N. Hurley-Walker, D. L. Kaplan, N. Barry,, A. P. Beardsley, M. E. Bell, G. Bernardi, J. D. Bowman, F. Briggs, J. R., Callingham, R. J. Cappallo, P. Carroll, A. A. Deshpande, J. S. Dillon, K. S., Dwarakanath, A. Ewall-Wice, L. Feng, B.-Q. For

TL;DR
This paper analyzes the radio-frequency interference environment of the Murchison Widefield Array, presents an automated RFI detection method, and offers recommendations to improve RFI mitigation for future radio telescopes like the SKA.
Contribution
It introduces an automated RFI detection strategy for the MWA, provides RFI statistics, and offers design recommendations for RFI mitigation in next-generation telescopes.
Findings
RFI detection removes 1.1% of data
Digital TV RFI occurs 3% of the time
MWA's remote location results in a cleaner RFI environment
Abstract
The Murchison Widefield Array (MWA) is a new low-frequency interferometric radio telescope built in Western Australia at one of the locations of the future Square Kilometre Array (SKA). We describe the automated radio-frequency interference (RFI) detection strategy implemented for the MWA, which is based on the AOFlagger platform, and present 72-231-MHz RFI statistics from 10 observing nights. RFI detection removes 1.1% of the data. RFI from digital TV (DTV) is observed 3% of the time due to occasional ionospheric or atmospheric propagation. After RFI detection and excision, almost all data can be calibrated and imaged without further RFI mitigation efforts, including observations within the FM and DTV bands. The results are compared to a previously published Low-Frequency Array (LOFAR) RFI survey. The remote location of the MWA results in a substantially cleaner RFI environment…
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