activity
20182022
most citedSKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge

72 citations · 152 across the 3 of their papers we have counts for

collaborators

12 papers

astro-ph.CO202225 cited

Detecting the power spectrum turnover with HI intensity mapping

Steven Cunnington

A goal for pathfinder intensity mapping (IM) surveys will be detecting features in the neutral hydrogen (HI) power spectrum, which serve as conclusive evidence of cosmological sign…

astro-ph.CO202172 cited

SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge

Marta Spinelli, Isabella P. Carucci, Steven Cunnington +5

Neutral Hydrogen Intensity Mapping (HI IM) surveys will be a powerful new probe of cosmology. However, strong astrophysical foregrounds contaminate the signal and their coupling wi…

astro-ph.CO2021

Gaussian Process Regression for foreground removal in HI intensity mapping experiments

Paula S. Soares, Catherine A. Watkinson, Steven Cunnington +1

We apply for the first time Gaussian Process Regression (GPR) as a foreground removal technique in the context of single-dish, low redshift HI intensity mapping, and present an ope…

astro-ph.CO2021

The HI intensity mapping bispectrum including observational effects

Steven Cunnington, Catherine Watkinson, Alkistis Pourtsidou

The bispectrum is a 3-point statistic with the potential to provide additional information beyond power spectra analyses of survey datasets. Radio telescopes which broadly survey t…

astro-ph.CO2020

HI intensity mapping with MeerKAT: Calibration pipeline for multi-dish autocorrelation observations

Jingying Wang, Mario G. Santos, Philip Bull +10

While most purpose-built 21cm intensity mapping experiments are close-packed interferometer arrays, general-purpose dish arrays should also be capable of measuring the cosmological…

astro-ph.CO2020

21cm foregrounds and polarization leakage: a user's guide on cleaning and mitigation strategies

Steven Cunnington, Melis O. Irfan, Isabella P. Carucci +2

The success of HI intensity mapping is largely dependent on how well 21cm foreground contamination can be controlled. In order to progress our understanding further, we present a r…