activity
20142020
most cited21CMMC: an MCMC analysis tool enabling astrophysical parameter studies of the cosmic 21 cm signal

247 citations · 827 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2020224 cited

Deep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations

Cathryn M. Trott, C. H. Jordan, S. Midgley +33

We compute the spherically-averaged power spectrum from four seasons of data obtained for the Epoch of Reionisation (EoR) project observed with the Murchison Widefield Array (MWA).…

astro-ph.IM201978 cited

Mitigating Internal Instrument Coupling II: A Method Demonstration with the Hydrogen Epoch of Reionization Array

Nicholas S. Kern, Aaron R. Parsons, Joshua S. Dillon +63

We present a study of internal reflection and cross coupling systematics in Phase I of the Hydrogen Epoch of Reionization Array (HERA). In a companion paper, we outlined the mathem…

astro-ph.IM2019141 cited

Improving the Epoch of Reionization Power Spectrum Results from Murchison Widefield Array Season 1 Observations

N. Barry, M. Wilensky, C. M. Trott +27

Measurements of 21 cm Epoch of Reionization (EoR) structure are subject to systematics originating from both the analysis and the observation conditions. Using 2013 data from the M…

astro-ph.CO20193 cited

Inference from the 21cm signal

Bradley Greig

Once we have a measurement, how do we extract this information from the signal? This chapter focusses on the inference of the interesting astrophysics and cosmology once we obtain…

astro-ph.IM201956 cited

Optimizing Sparse RFI Prediction using Deep Learning

Joshua Kerrigan, Paul La Plante, Saul Kohn +61

Radio Frequency Interference (RFI) is an ever-present limiting factor among radio telescopes even in the most remote observing locations. When looking to retain the maximum amount…

astro-ph.GA201654 cited

Quasar UV luminosity function evolution up to z=8

Serena Manti, Simona Gallerani, Andrea Ferrara +2

We study the redshift evolution of the quasar UV Luminosity Function (LF) for 0.5 < z < 6.5, by collecting the most up to date observational data and, in particular, the recently d…