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author Li, W.
Pober, J.C.
Barry, N.
Hazelton, B.J.
Morales, M.F.
Trott, Cathryn
Lanman, A.
Wilensky, M.
Sullivan, I.
Beardsley, A.P.
Booler, Tom
Bowman, J.D.
Byrne, R.
Crosse, B.
Emrich, David
Franzen, Thomas
Hasegawa, K.
Horsley, L.
Johnston-Hollitt, Melanie
Jacobs, D.C.
Jordan, Chris
Joseph, R.C.
Kaneuji, T.
Kaplan, D.L.
Kenney, David
Kubota, K.
Line, Jack
Lynch, Christene
McKinley, Ben
Mitchell, D.A.
Murray, Steven
Pallot, D.
Pindor, B.
Rahimi, M.
Riding, J.
Sleap, G.
Steele, K.
Takahashi, K.
Tingay, Steven
Walker, Mia
Wayth, Randall
Webster, R.L.
Williams, Andrew
Wu, C.
Wyithe, J.S.B.
Yoshiura, S.
Zheng, Q.
author_facet Li, W.
Pober, J.C.
Barry, N.
Hazelton, B.J.
Morales, M.F.
Trott, Cathryn
Lanman, A.
Wilensky, M.
Sullivan, I.
Beardsley, A.P.
Booler, Tom
Bowman, J.D.
Byrne, R.
Crosse, B.
Emrich, David
Franzen, Thomas
Hasegawa, K.
Horsley, L.
Johnston-Hollitt, Melanie
Jacobs, D.C.
Jordan, Chris
Joseph, R.C.
Kaneuji, T.
Kaplan, D.L.
Kenney, David
Kubota, K.
Line, Jack
Lynch, Christene
McKinley, Ben
Mitchell, D.A.
Murray, Steven
Pallot, D.
Pindor, B.
Rahimi, M.
Riding, J.
Sleap, G.
Steele, K.
Takahashi, K.
Tingay, Steven
Walker, Mia
Wayth, Randall
Webster, R.L.
Williams, Andrew
Wu, C.
Wyithe, J.S.B.
Yoshiura, S.
Zheng, Q.
author_sort Li, W.
building Curtin Institutional Repository
collection Online Access
description The compact configuration of Phase II of the Murchison Widefield Array (MWA) consists of both a redundant subarray and pseudo-random baselines, offering unique opportunities to perform sky-model and redundant interferometric calibration. The highly redundant hexagonal cores give improved power spectrum sensitivity. In this paper, we present the analysis of nearly 40 hr of data targeting one of the MWA's epoch of reionization (EoR) fields observed in 2016. We use both improved analysis techniques presented in Barry et al. and several additional techniques developed for this work, including data quality control methods and interferometric calibration approaches. We show the EoR power spectrum limits at redshift 6.5, 6.8, and 7.1 based on our deep analysis on this 40 hr data set. These limits span a range in k-space of 0.18 h Mpc-1 < k < 1.6 h Mpc-1, with a lowest measurement of Δ2 ≤ 2.39 × 103 mK2 at k = 0.59 h Mpc-1 and z = 6.5.
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institution Curtin University Malaysia
institution_category Local University
language English
last_indexed 2025-11-14T11:37:01Z
publishDate 2019
publisher IOP Publishing Ltd
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-915662023-05-16T07:05:56Z First Season MWA Phase II Epoch of Reionization Power Spectrum Results at Redshift 7 Li, W. Pober, J.C. Barry, N. Hazelton, B.J. Morales, M.F. Trott, Cathryn Lanman, A. Wilensky, M. Sullivan, I. Beardsley, A.P. Booler, Tom Bowman, J.D. Byrne, R. Crosse, B. Emrich, David Franzen, Thomas Hasegawa, K. Horsley, L. Johnston-Hollitt, Melanie Jacobs, D.C. Jordan, Chris Joseph, R.C. Kaneuji, T. Kaplan, D.L. Kenney, David Kubota, K. Line, Jack Lynch, Christene McKinley, Ben Mitchell, D.A. Murray, Steven Pallot, D. Pindor, B. Rahimi, M. Riding, J. Sleap, G. Steele, K. Takahashi, K. Tingay, Steven Walker, Mia Wayth, Randall Webster, R.L. Williams, Andrew Wu, C. Wyithe, J.S.B. Yoshiura, S. Zheng, Q. Science & Technology Physical Sciences Astronomy & Astrophysics BASE-LINE CALIBRATION INTERFEROMETRIC DATA COSMOLOGY MITEOR LIMITS ARRAY astro-ph.CO astro-ph.CO astro-ph.IM The compact configuration of Phase II of the Murchison Widefield Array (MWA) consists of both a redundant subarray and pseudo-random baselines, offering unique opportunities to perform sky-model and redundant interferometric calibration. The highly redundant hexagonal cores give improved power spectrum sensitivity. In this paper, we present the analysis of nearly 40 hr of data targeting one of the MWA's epoch of reionization (EoR) fields observed in 2016. We use both improved analysis techniques presented in Barry et al. and several additional techniques developed for this work, including data quality control methods and interferometric calibration approaches. We show the EoR power spectrum limits at redshift 6.5, 6.8, and 7.1 based on our deep analysis on this 40 hr data set. These limits span a range in k-space of 0.18 h Mpc-1 < k < 1.6 h Mpc-1, with a lowest measurement of Δ2 ≤ 2.39 × 103 mK2 at k = 0.59 h Mpc-1 and z = 6.5. 2019 Journal Article http://hdl.handle.net/20.500.11937/91566 10.3847/1538-4357/ab55e4 English https://arxiv.org/abs/1911.10216 http://purl.org/au-research/grants/arc/CE170100013 http://purl.org/au-research/grants/arc/FT180100321 http://purl.org/au-research/grants/arc/LE160100031 IOP Publishing Ltd restricted
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
BASE-LINE CALIBRATION
INTERFEROMETRIC DATA
COSMOLOGY
MITEOR
LIMITS
ARRAY
astro-ph.CO
astro-ph.CO
astro-ph.IM
Li, W.
Pober, J.C.
Barry, N.
Hazelton, B.J.
Morales, M.F.
Trott, Cathryn
Lanman, A.
Wilensky, M.
Sullivan, I.
Beardsley, A.P.
Booler, Tom
Bowman, J.D.
Byrne, R.
Crosse, B.
Emrich, David
Franzen, Thomas
Hasegawa, K.
Horsley, L.
Johnston-Hollitt, Melanie
Jacobs, D.C.
Jordan, Chris
Joseph, R.C.
Kaneuji, T.
Kaplan, D.L.
Kenney, David
Kubota, K.
Line, Jack
Lynch, Christene
McKinley, Ben
Mitchell, D.A.
Murray, Steven
Pallot, D.
Pindor, B.
Rahimi, M.
Riding, J.
Sleap, G.
Steele, K.
Takahashi, K.
Tingay, Steven
Walker, Mia
Wayth, Randall
Webster, R.L.
Williams, Andrew
Wu, C.
Wyithe, J.S.B.
Yoshiura, S.
Zheng, Q.
First Season MWA Phase II Epoch of Reionization Power Spectrum Results at Redshift 7
title First Season MWA Phase II Epoch of Reionization Power Spectrum Results at Redshift 7
title_full First Season MWA Phase II Epoch of Reionization Power Spectrum Results at Redshift 7
title_fullStr First Season MWA Phase II Epoch of Reionization Power Spectrum Results at Redshift 7
title_full_unstemmed First Season MWA Phase II Epoch of Reionization Power Spectrum Results at Redshift 7
title_short First Season MWA Phase II Epoch of Reionization Power Spectrum Results at Redshift 7
title_sort first season mwa phase ii epoch of reionization power spectrum results at redshift 7
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
BASE-LINE CALIBRATION
INTERFEROMETRIC DATA
COSMOLOGY
MITEOR
LIMITS
ARRAY
astro-ph.CO
astro-ph.CO
astro-ph.IM
url https://arxiv.org/abs/1911.10216
https://arxiv.org/abs/1911.10216
https://arxiv.org/abs/1911.10216
https://arxiv.org/abs/1911.10216
http://hdl.handle.net/20.500.11937/91566