Area of research
Astronomy and Astrophysics · Nuclear and High Energy Physics
Research interest
Research focused on Redshift and Murchison meteorite, with related work in Reionization, Remote sensing, Spectral density. Notable publications include 'The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies', 'wsclean: an implementation of a fast, generic wide-field imager for radio astronomy', and 'The Phase II Murchison Widefield Array: Design overview'.
GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic plane 345° <<i>l</i>< 67°, 180° <<i>l</i>< 240°
The Phase II Murchison Widefield Array: Design overview
Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWA
The spectral energy distribution of powerful starburst galaxies – I. Modelling the radio continuum
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
BROADBAND SPECTRAL MODELING OF THE EXTREME GIGAHERTZ-PEAKED SPECTRUM RADIO SOURCE PKS B0008-421
FOREGROUNDS IN WIDE-FIELD REDSHIFTED 21 cm POWER SPECTRA
UWA Profiles and Research Repository (University of Western Australia) 2015cited by 84position: middle
wsclean: an implementation of a fast, generic wide-field imager for radio astronomy
Modelling of the spectral energy distribution of Fornax A: leptonic and hadronic production of high-energy emission from the radio lobes
The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies
ON THE DETECTION AND TRACKING OF SPACE DEBRIS USING THE MURCHISON WIDEFIELD ARRAY. I. SIMULATIONS AND TEST OBSERVATIONS DEMONSTRATE FEASIBILITY