Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research focused on Redshift and Reionization, with related work in Field (mathematics), Spectral density, Spectral line. Notable publications include 'The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation', 'CHIPS: THE COSMOLOGICAL H i POWER SPECTRUM ESTIMATOR', and 'Empirical covariance modeling for 21 cm power spectrum estimation: A method demonstration and new limits from early Murchison Widefield Array 128-tile data'.
NSF-DOE Vera C. Rubin Observatory Observations of Interstellar Comet 3I/ATLAS (C/2025 N1)
COVID-19 and Preexisting Comorbidities: Risks, Synergies, and Clinical Outcomes
Understanding the diversity of 21 cm cosmology analyses
Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWA
The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array
CHIPS: THE COSMOLOGICAL H i POWER SPECTRUM ESTIMATOR
First limits on the 21 cm power spectrum during the Epoch of X-ray heating
THE IMPORTANCE OF WIDE-FIELD FOREGROUND REMOVAL FOR 21 cm COSMOLOGY: A DEMONSTRATION WITH EARLY MWA EPOCH OF REIONIZATION OBSERVATIONS
LOW-FREQUENCY OBSERVATIONS OF LINEARLY POLARIZED STRUCTURES IN THE INTERSTELLAR MEDIUM NEAR THE SOUTH GALACTIC POLE
Parametrizing Epoch of Reionization foregrounds: a deep survey of low-frequency point-source spectra with the Murchison Widefield Array
The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and Mitigation
Empirical covariance modeling for 21 cm power spectrum estimation: A method demonstration and new limits from early Murchison Widefield Array 128-tile data
CONFIRMATION OF WIDE-FIELD SIGNATURES IN REDSHIFTED 21 cm POWER SPECTRA
FOREGROUNDS IN WIDE-FIELD REDSHIFTED 21 cm POWER SPECTRA
UWA Profiles and Research Repository (University of Western Australia) 2015cited by 84position: middle
FAST HOLOGRAPHIC DECONVOLUTION: A NEW TECHNIQUE FOR PRECISION RADIO INTERFEROMETRY