activity
20122026
most citedDeep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations

224 citations · 1.1k across the 32 of their papers we have counts for

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28 papers · 1 filter

astro-ph.IM20252 cited

Determining Ideal Fields for Epoch of Reionisation Science Using the 21 cm Line

E. Jong, C. Trott, C. D. Nunhokee +1

The upcoming Square Kilometre Array Low Frequency (SKA-Low) interferometer will have the required sensitivity to detect the 21 cm line from neutral hydrogen during the Epoch of Rei…

astro-ph.IM2022

System design and calibration of SITARA -- a global 21 cm short spacing interferometer prototype

Jishnu N. Thekkeppattu, Benjamin McKinley, Cathryn M. Trott +2

Global 21-cm experiments require exquisitely precise calibration of the measurement systems in order to separate the weak 21-cm signal from Galactic and extragalactic foregrounds a…

astro-ph.IM2022

Imaging the Southern Sky at 159MHz using Spherical Harmonics with the Engineering Development Array 2

Michael A. Kriele, Randall B. Wayth, Mark J. Bentum +2

One of the major priorities of international radio astronomy is to study the early universe through the detection of the 21 cm HI line from the epoch of reionisation (EoR). Due to…

astro-ph.IM2021

Simulations of ionospheric refraction on radio interferometric data

J. Kariuki Chege, C. H. Jordan, C. Lynch +2

The Epoch of Reionisation (EoR) is the period within which the neutral universe transitioned to an ionised one. This period remains unobserved using low-frequency radio interferome…

astro-ph.IM2020

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.IM202022 cited

Modelling and peeling extended sources with shapelets: a Fornax A case study

J. L. B. Line, D. A. Mitchell, B. Pindor +6

To make a power spectrum (PS) detection of the 21 cm signal from the Epoch of Reionisation (EoR), one must avoid/subtract bright foreground sources. Sources such as Fornax A presen…