activity
20162021
most citedDeep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations

224 citations · 674 across the 12 of their papers we have counts for

collaborators

18 papers

astro-ph.CO20212 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.CO20217 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.CO202167 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

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.IM202116 cited

Dual Polarization Measurements of MWA Beampatterns at 137 MHz

A. Chokshi, J. L. B. Line, N. Barry +5

The wide adoption of low-frequency radio interferometers as a tool for deeper and higher resolution astronomical observations has revolutionised radio astronomy. Despite their cons…

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…