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

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 pro...

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Main 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
Format: Journal Article
Published: Cambridge University Press 2017
Online Access:http://hdl.handle.net/20.500.11937/57974
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author 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
author_facet 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
author_sort Lenc, E.
building Curtin Institutional Repository
collection Online Access
description 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.
first_indexed 2025-11-14T10:11:08Z
format Journal Article
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T10:11:08Z
publishDate 2017
publisher Cambridge University Press
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spelling curtin-20.500.11937-579742018-03-27T02:56:11Z The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array 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 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. 2017 Journal Article http://hdl.handle.net/20.500.11937/57974 10.1017/pasa.2017.36 Cambridge University Press fulltext
spellingShingle 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
The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array
title The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array
title_full The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array
title_fullStr The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array
title_full_unstemmed The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array
title_short The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array
title_sort challenges of low-frequency radio polarimetry: lessons from the murchison widefield array
url http://hdl.handle.net/20.500.11937/57974