activity
20162019
most citedFirst Season MWA Phase II EoR Power Spectrum Results at Redshift 7

98 citations · 216 across the 8 of their papers we have counts for

collaborators

8 papers

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.CO2019★ 9 cited

Detectability of 21cm signal during the Epoch of Reionization with 21cm-Lyman- emitter cross-correlation. III. Model dependence

Kenji Kubota, Akio. K. Inoue, Kenji Hasegawa +1

Detecting 21cm line in the intergalactic medium (IGM) during the Epoch of Reionization (EoR) suffers from foreground contamination such as Galactic synchrotron and extrag…

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…

astro-ph.CO2019★ 5 cited

Detectability of CMB Weak Lensing and HI Cross Correlation and constraints on cosmological parameters

Shoichiro Tanaka, Shintaro Yoshiura, Kenji Kubota +3

Neutral hydrogen (H) intensity mapping is capable of measuring redshift evolution of H density parameter , which is an important parameter to…

astro-ph.CO2017★ 14 cited

Detectability of 21cm-signal during the Epoch of Reionization with 21cm-Lyman-α emitter cross-correlation. II. Foreground contamination

S. Yoshiura, J. L. B. Line, K. Kubota +2

Cross-correlation between the redshifted 21 cm signal and Lyman-α emitters (LAEs) is powerful tool to probe the Epoch of Reionization (EoR). Although the cross-power spectrum (PS)…

astro-ph.CO2017★ 30 cited

Detectability of 21cm-signal during the Epoch of Reionization with 21cm-Lyman- emitter cross-correlation. I

Kenji Kubota, Shintaro Yoshiura, Keitaro Takahashi +5

Detection of the redshifted 21cm-line signal from neutral hydrogen in the intergalactic medium (IGM) during the Epoch of Reionization (EoR) is complicated by intense foregrounds su…

astro-ph.CO2016★ 21 cited

Expected constraints on models of the epoch of reionization with the variance and skewness in redshifted 21cm-line fluctuations

Kenji Kubota, Shintaro Yoshiura, Hayato Shimabukuro +1

Redshifted 21cm-line signal from neutral hydrogens in the intergalactic medium (IGM) gives a direct probe of the epoch of reionization (EoR). In this paper, we investigate the pote…