activity
20232026
most citedHydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning

33 citations · 71 across the 21 of their papers we have counts for

collaborators
Showing 2024Show all

10 papers · 1 filter

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.IM2024★ 10 cited

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.IM2024★ 2 cited

Mitigating calibration errors from mutual coupling with time-domain filtering of 21 cm cosmological radio observations

N. Charles, N. S. Kern, R. Pascua +80

The 21 cm transition from neutral Hydrogen promises to be the best observational probe of the Epoch of Reionisation (EoR). This has led to the construction of low-frequency radio i…

astro-ph.CO2024★ 2 cited

Modes of the Dark Ages 21cm field accessible to a lunar radio interferometer

Philip Bull, Caroline Guandalin, Chris Addis

At redshifts beyond , the 21cm line from neutral hydrogen is expected to be essentially the only viable probe of the 3D matter distribution. The lunar far-side is an…

astro-ph.CO2024★ 6 cited

Sensitivity of Bayesian 21 cm power spectrum estimation to foreground model errors

Jacob Burba, Philip Bull, Michael J. Wilensky +3

Power spectrum estimators are an important tool in efforts to detect the 21 cm brightness temperature fluctuations from neutral hydrogen at early times. An initial detection will l…

astro-ph.IM2024★ 1 cited

High-dimensional inference of radio interferometer beam patterns I: Parametric model of the HERA beams

Michael J. Wilensky, Jacob Burba, Philip Bull +6

Accurate modelling of the primary beam is an important but difficult task in radio astronomy. For high dynamic range problems such as 21cm intensity mapping, small modelling errors…

astro-ph.CO2024★ 1 cited

Disentangling the anisotropic radio sky: Fisher forecasts for 21cm arrays

Zheng Zhang, Philip Bull, Katrine A. Glasscock

The existence of a radio synchrotron background (RSB) excess is implied by a number of measurements, including excess emission seen by the ARCADE~2 and LWA experiments. Highly sens…

astro-ph.IM2024★ 5 cited

Statistical estimation of full-sky radio maps from 21cm array visibility data using Gaussian constrained realizations

Katrine A. Glasscock, Philip Bull, Jacob Burba +2

An important application of next-generation wide-field radio interferometers is making high dynamic range maps of radio emission. Traditional deconvolution methods like CLEAN can g…

astro-ph.CO2024★ 1 cited

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.IM2024★ 33 cited

Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning

Lindsay M. Berkhout, Daniel C. Jacobs, Zuhra Abdurashidova +93

This paper presents the design and deployment of the Hydrogen Epoch of Reionization Array (HERA) phase II system. HERA is designed as a staged experiment targeting 21 cm emission m…