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The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array

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Authors
Lenc, E.
Anderson, C.
Barry, N.
Bowman, J.
Cairns, I.
Farnes, J.
Gaensler, B.
Heald, G.
Johnston-Hollitt, M.
Kaplan, D.
Lynch, C.
McCauley, P.
Mitchell, D.
Morgan, John
Morales, M.
Murphy, T.
Offringa, A.
Ord, S.
Pindor, B.
Riseley, C.
Sadler, E.
Sobey, Charlotte
Sokolowski, Marcin
Sullivan, I.
O Sullivan, S.
Sun, X.
Tremblay, S.
Trott, Cathryn
Wayth, Randall
Date
2017
Type
Journal Article

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Lenc, E. and Anderson, C. and Barry, N. and Bowman, J. and Cairns, I. and Farnes, J. and Gaensler, B. et al. 2017. The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array. Publications of the Astronomical Society of Australia. 34: e040.
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Publications of the Astronomical Society of Australia
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Curtin Institute of Radio Astronomy (Physics)
Remarks

This paper has been accepted for publication and will appear in a revised form, subsequent to peer review and/or editorial input by Cambridge University Press, in Publications of the Astronomical Society of Australia published by Cambridge University Press. Copyright © 2017 Astronomical Society of Australia.

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Abstract

We present techniques developed to calibrate and correct Murchison Widefield Array low-frequency (72–300 MHz) radio observations for polarimetry. The extremely wide field-of-view, excellent instantaneous (u, v)-coverage and sensitivity to degree-scale structure that the Murchison Widefield Array provides enable instrumental calibration, removal of instrumental artefacts, and correction for ionospheric Faraday rotation through imaging techniques. With the demonstrated polarimetric capabilities of the Murchison Widefield Array, we discuss future directions for polarimetric science at low frequencies to answer outstanding questions relating to polarised source counts, source depolarisation, pulsar science, low-mass stars, exoplanets, the nature of the interstellar and intergalactic media, and the solar environment.