most citedA Generalized Method for Characterizing 21-cm Power Spectrum Signal Loss from Temporal Filtering of Drift-scanning Visibilities

1 citations · 1 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2025

First Results from HERA Phase II

The HERA Collaboration, Zuhra Abdurashidova, Tyrone Adams +83

We report the first upper limits on the power spectrum of 21-cm fluctuations during the Epoch of Reionization and Cosmic Dawn from Phase II of the Hydrogen Epoch of Reionization Ar…

astro-ph.CO2025

Systematic assessment of the Hubble tension via Bayesian jackknife testing

Thomas Hughes, Michael J. Wilensky, Philip Bull

Statistically-significant differences in the value of the Hubble parameter are found depending on the measurement method that is used, a result known as the Hubble tension. A varie…

astro-ph.IM2025

High Dimensional Beam Inference II: Inference of a Perturbed HERA Beam from Simulated Visibility Data

Michael J. Wilensky, Philip Bull, Nicolas Fagnoni

Accurate beam modeling is important in many radio astronomy applications. In this paper, we focus on beam modeling for 21-cm intensity mapping experiments using radio interferomete…

astro-ph.CO2024

Impacts and Statistical Mitigation of Missing Data on the 21cm Power Spectrum: A Case Study with the Hydrogen Epoch of Reionization Array

Kai-Feng Chen, Michael J. Wilensky, Adrian Liu +66

The precise characterization and mitigation of systematic effects is one of the biggest roadblocks impeding the detection of the fluctuations of cosmological 21cm signals. Missing…

astro-ph.CO20241 cited

A Generalized Method for Characterizing 21-cm Power Spectrum Signal Loss from Temporal Filtering of Drift-scanning Visibilities

Robert Pascua, Zachary E. Martinot, Adrian Liu +7

A successful detection of the cosmological 21-cm signal from intensity mapping experiments (for example, during the Epoch of Reioinization or Cosmic Dawn) is contingent on the supp…

astro-ph.IM2024

RHINO: A large horn antenna for detecting the 21cm global signal

Philip Bull, Ahmed El-Makadema, Hugh Garsden +11

The sky-averaged brightness temperature of the 21cm line from neutral hydrogen provides a sensitive probe of the thermal state of the intergalactic medium, particularly before and…