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author Trott, Cathryn
Watkinson, C.A.
Jordan, Chris
Yoshiura, S.
Majumdar, S.
Barry, Nichole
Byrne, R.
Hazelton, B.J.
Hasegawa, K.
Joseph, R.
Kaneuji, T.
Kubota, K.
Li, W.
Line, Jack
Lynch, Christene
McKinley, Ben
Mitchell, D.A.
Morales, M.F.
Murray, Steven
Pindor, B.
Pober, J.C.
Rahimi, M.
Riding, J.
Takahashi, K.
Tingay, Steven
Wayth, Randall
Webster, R.L.
Wilensky, M.
Wyithe, J.S.B.
Zheng, Q.
Emrich, David
Beardsley, A.P.
Booler, Tom
Crosse, B.
Franzen, Thomas
Horsley, L.
Johnston-Hollitt, Melanie
Kaplan, D.L.
Kenney, David
Pallot, D.
Sleap, G.
Steele, K.
Walker, Mia
Williams, Andrew
Wu, C.
author_facet Trott, Cathryn
Watkinson, C.A.
Jordan, Chris
Yoshiura, S.
Majumdar, S.
Barry, Nichole
Byrne, R.
Hazelton, B.J.
Hasegawa, K.
Joseph, R.
Kaneuji, T.
Kubota, K.
Li, W.
Line, Jack
Lynch, Christene
McKinley, Ben
Mitchell, D.A.
Morales, M.F.
Murray, Steven
Pindor, B.
Pober, J.C.
Rahimi, M.
Riding, J.
Takahashi, K.
Tingay, Steven
Wayth, Randall
Webster, R.L.
Wilensky, M.
Wyithe, J.S.B.
Zheng, Q.
Emrich, David
Beardsley, A.P.
Booler, Tom
Crosse, B.
Franzen, Thomas
Horsley, L.
Johnston-Hollitt, Melanie
Kaplan, D.L.
Kenney, David
Pallot, D.
Sleap, G.
Steele, K.
Walker, Mia
Williams, Andrew
Wu, C.
author_sort Trott, Cathryn
building Curtin Institutional Repository
collection Online Access
description We apply two methods to estimate the 21-cm bispectrum from data taken within the Epoch of Reionisation (EoR) project of the Murchison Widefield Array (MWA). Using data acquired with the Phase II compact array allows a direct bispectrum estimate to be undertaken on the multiple redundantly spaced triangles of antenna tiles, as well as an estimate based on data gridded to the uv-plane. The direct and gridded bispectrum estimators are applied to 21 h of high-band (167-197 MHz; z = 6.2-7.5) data from the 2016 and 2017 observing seasons. Analytic predictions for the bispectrum bias and variance for point-source foregrounds are derived. We compare the output of these approaches, the foreground contribution to the signal, and future prospects for measuring the bispectra with redundant and non-redundant arrays. We find that some triangle configurations yield bispectrum estimates that are consistent with the expected noise level after 10 h, while equilateral configurations are strongly foreground-dominated. Careful choice of triangle configurations may be made to reduce foreground bias that hinders power spectrum estimators, and the 21-cm bispectrum may be accessible in less time than the 21-cm power spectrum for some wave modes, with detections in hundreds of hours.
first_indexed 2025-11-14T11:37:05Z
format Journal Article
id curtin-20.500.11937-91578
institution Curtin University Malaysia
institution_category Local University
language English
last_indexed 2025-11-14T11:37:05Z
publishDate 2019
publisher CAMBRIDGE UNIV PRESS
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-915782023-05-16T03:16:26Z Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array Trott, Cathryn Watkinson, C.A. Jordan, Chris Yoshiura, S. Majumdar, S. Barry, Nichole Byrne, R. Hazelton, B.J. Hasegawa, K. Joseph, R. Kaneuji, T. Kubota, K. Li, W. Line, Jack Lynch, Christene McKinley, Ben Mitchell, D.A. Morales, M.F. Murray, Steven Pindor, B. Pober, J.C. Rahimi, M. Riding, J. Takahashi, K. Tingay, Steven Wayth, Randall Webster, R.L. Wilensky, M. Wyithe, J.S.B. Zheng, Q. Emrich, David Beardsley, A.P. Booler, Tom Crosse, B. Franzen, Thomas Horsley, L. Johnston-Hollitt, Melanie Kaplan, D.L. Kenney, David Pallot, D. Sleap, G. Steele, K. Walker, Mia Williams, Andrew Wu, C. Science & Technology Physical Sciences Astronomy & Astrophysics cosmology early universe instrumentation methods statistical NON-GAUSSIANITY 21-CM COSMOLOGY astro-ph.CO astro-ph.CO astro-ph.IM We apply two methods to estimate the 21-cm bispectrum from data taken within the Epoch of Reionisation (EoR) project of the Murchison Widefield Array (MWA). Using data acquired with the Phase II compact array allows a direct bispectrum estimate to be undertaken on the multiple redundantly spaced triangles of antenna tiles, as well as an estimate based on data gridded to the uv-plane. The direct and gridded bispectrum estimators are applied to 21 h of high-band (167-197 MHz; z = 6.2-7.5) data from the 2016 and 2017 observing seasons. Analytic predictions for the bispectrum bias and variance for point-source foregrounds are derived. We compare the output of these approaches, the foreground contribution to the signal, and future prospects for measuring the bispectra with redundant and non-redundant arrays. We find that some triangle configurations yield bispectrum estimates that are consistent with the expected noise level after 10 h, while equilateral configurations are strongly foreground-dominated. Careful choice of triangle configurations may be made to reduce foreground bias that hinders power spectrum estimators, and the 21-cm bispectrum may be accessible in less time than the 21-cm power spectrum for some wave modes, with detections in hundreds of hours. 2019 Journal Article http://hdl.handle.net/20.500.11937/91578 10.1017/pasa.2019.15 English https://arxiv.org/abs/1905.07161 http://purl.org/au-research/grants/arc/CE170100013 http://purl.org/au-research/grants/arc/FT180100196 http://purl.org/au-research/grants/arc/LE160100031 CAMBRIDGE UNIV PRESS restricted
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
cosmology
early universe
instrumentation
methods
statistical
NON-GAUSSIANITY
21-CM
COSMOLOGY
astro-ph.CO
astro-ph.CO
astro-ph.IM
Trott, Cathryn
Watkinson, C.A.
Jordan, Chris
Yoshiura, S.
Majumdar, S.
Barry, Nichole
Byrne, R.
Hazelton, B.J.
Hasegawa, K.
Joseph, R.
Kaneuji, T.
Kubota, K.
Li, W.
Line, Jack
Lynch, Christene
McKinley, Ben
Mitchell, D.A.
Morales, M.F.
Murray, Steven
Pindor, B.
Pober, J.C.
Rahimi, M.
Riding, J.
Takahashi, K.
Tingay, Steven
Wayth, Randall
Webster, R.L.
Wilensky, M.
Wyithe, J.S.B.
Zheng, Q.
Emrich, David
Beardsley, A.P.
Booler, Tom
Crosse, B.
Franzen, Thomas
Horsley, L.
Johnston-Hollitt, Melanie
Kaplan, D.L.
Kenney, David
Pallot, D.
Sleap, G.
Steele, K.
Walker, Mia
Williams, Andrew
Wu, C.
Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array
title Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array
title_full Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array
title_fullStr Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array
title_full_unstemmed Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array
title_short Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array
title_sort gridded and direct epoch of reionisation bispectrum estimates using the murchison widefield array
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
cosmology
early universe
instrumentation
methods
statistical
NON-GAUSSIANITY
21-CM
COSMOLOGY
astro-ph.CO
astro-ph.CO
astro-ph.IM
url https://arxiv.org/abs/1905.07161
https://arxiv.org/abs/1905.07161
https://arxiv.org/abs/1905.07161
https://arxiv.org/abs/1905.07161
http://hdl.handle.net/20.500.11937/91578