The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation

The Murchison Widefield Array is a new low-frequency interferometric radio telescope built in Western Australia at one of the locations of the future Square Kilometre Array. We describe the automated radio-frequency interference detection strategy implemented for the Murchison Widefield Array, which...

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Main Authors: Lonsdale, Colin John, McWhirter, Stephen R., Dillon, Joshua Shane, Ewall-Wice, Aaron Michael, Feng, Lu, Neben, Abraham Richard, Tegmark, Max Erik, Williams, Christopher Leigh, Cappallo, Roger J, Hewitt, Jacqueline N, Morgan, Edward H
Other Authors: Haystack Observatory
Format: Article
Language:en_US
Published: CSIRO Publishing 2015
Online Access:http://hdl.handle.net/1721.1/98050
https://orcid.org/0000-0002-4117-570X
https://orcid.org/0000-0001-7776-7240
https://orcid.org/0000-0001-7130-208X
https://orcid.org/0000-0002-0086-7363
https://orcid.org/0000-0003-3336-9958
https://orcid.org/0000-0001-7670-7190
https://orcid.org/0000-0003-0422-2324
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author Lonsdale, Colin John
McWhirter, Stephen R.
Dillon, Joshua Shane
Ewall-Wice, Aaron Michael
Feng, Lu
Neben, Abraham Richard
Tegmark, Max Erik
Williams, Christopher Leigh
Cappallo, Roger J
Hewitt, Jacqueline N
Morgan, Edward H
author2 Haystack Observatory
author_facet Haystack Observatory
Lonsdale, Colin John
McWhirter, Stephen R.
Dillon, Joshua Shane
Ewall-Wice, Aaron Michael
Feng, Lu
Neben, Abraham Richard
Tegmark, Max Erik
Williams, Christopher Leigh
Cappallo, Roger J
Hewitt, Jacqueline N
Morgan, Edward H
author_sort Lonsdale, Colin John
collection MIT
description The Murchison Widefield Array is a new low-frequency interferometric radio telescope built in Western Australia at one of the locations of the future Square Kilometre Array. We describe the automated radio-frequency interference detection strategy implemented for the Murchison Widefield Array, which is based on the aoflagger platform, and present 72–231 MHz radio-frequency interference statistics from 10 observing nights. Radio-frequency interference detection removes 1.1% of the data. Radio-frequency interference from digital TV is observed 3% of the time due to occasional ionospheric or atmospheric propagation. After radio-frequency interference detection and excision, almost all data can be calibrated and imaged without further radio-frequency interference mitigation efforts, including observations within the FM and digital TV bands. The results are compared to a previously published Low-Frequency Array radio-frequency interference survey. The remote location of the Murchison Widefield Array results in a substantially cleaner radio-frequency interference environment compared to Low-Frequency Array’s radio environment, but adequate detection of radio-frequency interference is still required before data can be analysed. We include specific recommendations designed to make the Square Kilometre Array more robust to radio-frequency interference, including: the availability of sufficient computing power for radio-frequency interference detection; accounting for radio-frequency interference in the receiver design; a smooth band-pass response; and the capability of radio-frequency interference detection at high time and frequency resolution (second and kHz-scale respectively).
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spelling mit-1721.1/980502022-10-02T01:47:19Z The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation Lonsdale, Colin John McWhirter, Stephen R. Dillon, Joshua Shane Ewall-Wice, Aaron Michael Feng, Lu Neben, Abraham Richard Tegmark, Max Erik Williams, Christopher Leigh Cappallo, Roger J Hewitt, Jacqueline N Morgan, Edward H Haystack Observatory MIT Kavli Institute for Astrophysics and Space Research Cappallo, Roger J. Lonsdale, Colin John McWhirter, Stephen R. Dillon, Joshua Shane Ewall-Wice, Aaron Michael Feng, Lu Hewitt, Jacqueline N. Morgan, Edward H. Neben, Abraham Richard Tegmark, Max Erik Williams, Christopher Leigh The Murchison Widefield Array is a new low-frequency interferometric radio telescope built in Western Australia at one of the locations of the future Square Kilometre Array. We describe the automated radio-frequency interference detection strategy implemented for the Murchison Widefield Array, which is based on the aoflagger platform, and present 72–231 MHz radio-frequency interference statistics from 10 observing nights. Radio-frequency interference detection removes 1.1% of the data. Radio-frequency interference from digital TV is observed 3% of the time due to occasional ionospheric or atmospheric propagation. After radio-frequency interference detection and excision, almost all data can be calibrated and imaged without further radio-frequency interference mitigation efforts, including observations within the FM and digital TV bands. The results are compared to a previously published Low-Frequency Array radio-frequency interference survey. The remote location of the Murchison Widefield Array results in a substantially cleaner radio-frequency interference environment compared to Low-Frequency Array’s radio environment, but adequate detection of radio-frequency interference is still required before data can be analysed. We include specific recommendations designed to make the Square Kilometre Array more robust to radio-frequency interference, including: the availability of sufficient computing power for radio-frequency interference detection; accounting for radio-frequency interference in the receiver design; a smooth band-pass response; and the capability of radio-frequency interference detection at high time and frequency resolution (second and kHz-scale respectively). 2015-08-07T13:12:21Z 2015-08-07T13:12:21Z 2015-03 2014-12 Article http://purl.org/eprint/type/JournalArticle 1323-3580 1448-6083 http://hdl.handle.net/1721.1/98050 Offringa, A. R., R. B. Wayth, N. Hurley-Walker, D. L. Kaplan, N. Barry, A. P. Beardsley, M. E. Bell, et al. “The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation.” Publications of the Astronomical Society of Australia 32 (2015). https://orcid.org/0000-0002-4117-570X https://orcid.org/0000-0001-7776-7240 https://orcid.org/0000-0001-7130-208X https://orcid.org/0000-0002-0086-7363 https://orcid.org/0000-0003-3336-9958 https://orcid.org/0000-0001-7670-7190 https://orcid.org/0000-0003-0422-2324 en_US http://dx.doi.org/10.1017/pasa.2015.7 Publications of the Astronomical Society of Australia Creative Commons Attribution-Noncommercial-Share Alike http://creativecommons.org/licenses/by-nc-sa/4.0/ application/pdf CSIRO Publishing arXiv
spellingShingle Lonsdale, Colin John
McWhirter, Stephen R.
Dillon, Joshua Shane
Ewall-Wice, Aaron Michael
Feng, Lu
Neben, Abraham Richard
Tegmark, Max Erik
Williams, Christopher Leigh
Cappallo, Roger J
Hewitt, Jacqueline N
Morgan, Edward H
The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation
title The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation
title_full The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation
title_fullStr The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation
title_full_unstemmed The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation
title_short The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation
title_sort low frequency environment of the murchison widefield array radio frequency interference analysis and mitigation
url http://hdl.handle.net/1721.1/98050
https://orcid.org/0000-0002-4117-570X
https://orcid.org/0000-0001-7776-7240
https://orcid.org/0000-0001-7130-208X
https://orcid.org/0000-0002-0086-7363
https://orcid.org/0000-0003-3336-9958
https://orcid.org/0000-0001-7670-7190
https://orcid.org/0000-0003-0422-2324
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