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...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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格式: | Journal article |
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Cambridge University Press
2017
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_version_ | 1826292661240201216 |
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author | Lenc, E Anderson, CS Barry, N Bowman, JD Cairns, IH Farnes, JS Gaensler, BM Heald, G Johnston-Hollitt, M Kaplan, DL Lynch, CR McCauley, PI Mitchell, DA Morgan, J Morales, MF Murphy, T Offringa, AR Ord, SM Pindor, B Riseley, C Sadler, EM Sobey, C Sokolowski, M Sullivan, IS O’Sullivan, SP Sun, XH Tremblay, SE Trott, CM Wayth, RB |
author_facet | Lenc, E Anderson, CS Barry, N Bowman, JD Cairns, IH Farnes, JS Gaensler, BM Heald, G Johnston-Hollitt, M Kaplan, DL Lynch, CR McCauley, PI Mitchell, DA Morgan, J Morales, MF Murphy, T Offringa, AR Ord, SM Pindor, B Riseley, C Sadler, EM Sobey, C Sokolowski, M Sullivan, IS O’Sullivan, SP Sun, XH Tremblay, SE Trott, CM Wayth, RB |
author_sort | Lenc, E |
collection | OXFORD |
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 | 2024-03-07T03:18:08Z |
format | Journal article |
id | oxford-uuid:b6832be8-08b1-41d5-9dc7-b70813ca4e47 |
institution | University of Oxford |
last_indexed | 2024-03-07T03:18:08Z |
publishDate | 2017 |
publisher | Cambridge University Press |
record_format | dspace |
spelling | oxford-uuid:b6832be8-08b1-41d5-9dc7-b70813ca4e472022-03-27T04:41:31ZThe challenges of low-frequency radio polarimetry: Lessons from the Murchison widefield arrayJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:b6832be8-08b1-41d5-9dc7-b70813ca4e47Symplectic Elements at OxfordCambridge University Press2017Lenc, EAnderson, CSBarry, NBowman, JDCairns, IHFarnes, JSGaensler, BMHeald, GJohnston-Hollitt, MKaplan, DLLynch, CRMcCauley, PIMitchell, DAMorgan, JMorales, MFMurphy, TOffringa, AROrd, SMPindor, BRiseley, CSadler, EMSobey, CSokolowski, MSullivan, ISO’Sullivan, SPSun, XHTremblay, SETrott, CMWayth, RBWe 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. |
spellingShingle | Lenc, E Anderson, CS Barry, N Bowman, JD Cairns, IH Farnes, JS Gaensler, BM Heald, G Johnston-Hollitt, M Kaplan, DL Lynch, CR McCauley, PI Mitchell, DA Morgan, J Morales, MF Murphy, T Offringa, AR Ord, SM Pindor, B Riseley, C Sadler, EM Sobey, C Sokolowski, M Sullivan, IS O’Sullivan, SP Sun, XH Tremblay, SE Trott, CM Wayth, RB 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 |
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