collaborators

9 papers

astro-ph.IM2025

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…

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.CO2025

A demonstration of the effect of fringe-rate filtering in the Hydrogen Epoch of Reionization Array delay power spectrum pipeline

Hugh Garsden, Philip Bull, Mike Wilensky +94

Radio interferometers targeting the 21cm brightness temperature fluctuations at high redshift are subject to systematic effects that operate over a range of different timescales. T…

astro-ph.CO2025

Bayesian evidence for flux scale errors in Galactic synchrotron maps

Michael J. Wilensky, Melis O. Irfan, Philip Bull

The 408 MHz Haslam map is widely used as a low-frequency anchor for the intensity and morphology of Galactic synchrotron emission. Multi-frequency, multi-experiment fits show evide…