activity
20192026
most citedDeep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations

224 citations · 975 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.CO2026

Bayesian power spectrum estimation with modelling of systematic effects in delay-fringe rate space

Sohini Dutta, Philip Bull, Jacob Burba +3

Observing the Epoch of Reionisation using 21cm radio interferometry has proven to be a challenging task. Extraction of the extremely faint redshifted signal is complicated by the p…

astro-ph.IM2024★ 2 cited

Mitigating calibration errors from mutual coupling with time-domain filtering of 21 cm cosmological radio observations

N. Charles, N. S. Kern, R. Pascua +80

The 21 cm transition from neutral Hydrogen promises to be the best observational probe of the Epoch of Reionisation (EoR). This has led to the construction of low-frequency radio i…

astro-ph.CO2024★ 4 cited

Investigating Mutual Coupling in the Hydrogen Epoch of Reionization Array and Mitigating its Effects on the 21-cm Power Spectrum

E. Rath, R. Pascua, A. T. Josaitis +78

Interferometric experiments designed to detect the highly redshifted 21-cm signal from neutral hydrogen are producing increasingly stringent constraints on the 21-cm power spectrum…

astro-ph.CO2023★ 19 cited

Evidence of Ultra-faint Radio Frequency Interference in Deep 21~cm Epoch of Reionization Power Spectra with the Murchison Widefield Array

Michael J. Wilensky, Miguel F. Morales, Bryna J. Hazelton +7

We present deep upper limits from the 2014 Murchison Widefield Array (MWA) Phase I observing season, with a particular emphasis on identifying the spectral fingerprints of extremel…

astro-ph.CO2022★ 7 cited

Why and When to Expect Gaussian Error Distributions in Epoch of Reionization 21-cm Power Spectrum Measurements

Michael J. Wilensky, Jordan Brown, Bryna J. Hazelton

We explore error distributions in Epoch of Reionization 21-cm power spectrum estimators using a combination of mathematical analysis and numerical simulations. We provide closed fo…

astro-ph.CO2022★ 22 cited

Statistical recovery of 21cm visibilities and their power spectra with Gaussian constrained realisations and Gibbs sampling

Fraser Kennedy, Philip Bull, Michael Wilensky +2

Radio interferometers designed to probe the 21cm signal from Cosmic Dawn and the Epoch of Reionisation must contend with systematic effects that make it difficult to achieve suffic…

astro-ph.IM2022★ 4 cited

Bayesian jackknife tests with a small number of subsets: Application to HERA 21cm power spectrum upper limits

Michael J. Wilensky, Fraser Kennedy, Philip Bull +2

We present a Bayesian jackknife test for assessing the probability that a data set contains biased subsets, and, if so, which of the subsets are likely to be biased. The test can b…

astro-ph.CO2022★ 184 cited

Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations

The HERA Collaboration, Zara Abdurashidova, Tyrone Adams +92

We report the most sensitive upper limits to date on the 21 cm epoch of reionization power spectrum using 94 nights of observing with Phase I of the Hydrogen Epoch of Reionization…

astro-ph.CO2021★ 2 cited

Epoch of Reionization Power Spectrum Limits from Murchison Widefield Array Data Targeted at EoR1 Field

M. Rahimi, B. Pindor, J. L. B. Line +28

Current attempts to measure the 21cm Power Spectrum of neutral hydrogen during the Epoch of Reionization are limited by systematics which produce measured upper limits above both t…

astro-ph.IM2021★ 14 cited

Exploring the consequences of chromatic data excision in 21-cm Epoch of Reionization power spectrum observations

Michael J. Wilensky, Bryna J. Hazelton, Miguel F. Morales

We explore how chromatic RFI flags affect 21-cm power spectrum measurements. We particularly study flags that are coarser than the analysis resolution. We find that such RFI flags…

astro-ph.CO2021★ 7 cited

Constraining the 21cm brightness temperature of the IGM at =6.6 around LAEs with the Murchison Widefield Array

Cathryn M. Trott, C. H. Jordan, J. L. B. Line +29

The locations of Ly- emitting galaxies (LAEs) at the end of the Epoch of Reionisation (EoR) are expected to correlate with regions of ionised hydrogen, traced by the redshifted…

astro-ph.CO2021★ 67 cited

A new MWA limit on the 21 cm Power Spectrum at Redshifts 13 17

S. Yoshiura, B. Pindor, J. L. B. Line +29

Observations in the lowest MWA band between MHz have the potential to constrain the distribution of neutral hydrogen in the intergalactic medium at redshift .…

astro-ph.IM2021

A Real Time Processing System for Big Data in Astronomy: Applications to HERA

Paul La Plante, Peter K. G. Williams, Matthew Kolopanis +72

As current- and next-generation astronomical instruments come online, they will generate an unprecedented deluge of data. Analyzing these data in real time presents unique conceptu…

astro-ph.IM2020★ 10 cited

The Impact of Tandem Redundant/Sky-Based Calibration in MWA Phase II Data Analysis

Zheng Zhang, Jonathan C. Pober, Wenyang Li +26

Precise instrumental calibration is of crucial importance to 21-cm cosmology experiments. The Murchison Widefield Array's (MWA) Phase II compact configuration offers us opportuniti…

astro-ph.IM2020★ 37 cited

A Unified Calibration Framework for 21 cm Cosmology

Ruby Byrne, Miguel F. Morales, Bryna Hazelton +1

Calibration precision is currently a limiting systematic in 21 cm cosmology experiments. While there are innumerable calibration approaches, most can be categorized as either `sky-…

astro-ph.IM2020★ 29 cited

Quantifying Excess Power from Radio Frequency Interference in Epoch of Reionization Measurements

Michael J. Wilensky, Nichole Barry, Miguel F. Morales +2

We quantify the effect of radio frequency interference (RFI) on measurements of the 21-cm power spectrum during the Epoch of Reionization (EoR). Specifically, we investigate how th…

astro-ph.CO2020★ 224 cited

Deep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations

Cathryn M. Trott, C. H. Jordan, S. Midgley +33

We compute the spherically-averaged power spectrum from four seasons of data obtained for the Epoch of Reionisation (EoR) project observed with the Murchison Widefield Array (MWA).…

astro-ph.CO2019★ 98 cited

First Season MWA Phase II EoR Power Spectrum Results at Redshift 7

W. Li, J. C. Pober, N. Barry +44

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 per…

astro-ph.IM2019★ 141 cited

Improving the Epoch of Reionization Power Spectrum Results from Murchison Widefield Array Season 1 Observations

N. Barry, M. Wilensky, C. M. Trott +27

Measurements of 21 cm Epoch of Reionization (EoR) structure are subject to systematics originating from both the analysis and the observation conditions. Using 2013 data from the M…

astro-ph.IM2019★ 65 cited

Absolving the SSINS of Precision Interferometric Radio Data: A New Technique for Mitigating Faint Radio Frequency Interference

Michael J. Wilensky, Miguel F. Morales, Bryna J. Hazelton +3

We introduce a new pipeline for analyzing and mitigating radio frequency interference (RFI), which we call Sky-Subtracted Incoherent Noise Spectra (SSINS). SSINS is designed to ide…

astro-ph.CO2019★ 32 cited

Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield Array

Cathryn M. Trott, Catherine A. Watkinson, Christopher H. Jordan +42

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 wit…

astro-ph.CO2019★ 7 cited

Robust statistics toward detection of the 21 cm signal from the Epoch of Reionisation

Cathryn M. Trott, Shih Ching Fu, Steven Murray +26

We explore methods for robust estimation of the 21 cm signal from the Epoch of Reionisation (EoR). A Kernel Density Estimator (KDE) is introduced for measuring the spatial temperat…