Area of research
Astronomy and Astrophysics · Nuclear and High Energy Physics
Research interest
Research interests include Radio Astronomy Observations and Technology, Astrophysics and Cosmic Phenomena, Antenna Design and Optimization, and Galaxies: Formation, Evolution, Phenomena.
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
No Low-frequency Emission from Extremely Bright Fast Radio Bursts
Low Altitude Solar Magnetic Reconnection, Type III Solar Radio Bursts, and X-ray Emissions
The Challenges of Low-Frequency Radio Polarimetry: Lessons from the Murchison Widefield Array
The spectral energy distribution of powerful starburst galaxies – I. Modelling the radio continuum
GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey – I. A low-frequency extragalactic catalogue
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
Limits on Fast Radio Bursts and other transient sources at 182 MHz using the Murchison Widefield Array
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 154 MHz radio sky observed by the Murchison Widefield Array: noise, confusion, and first source count analyses
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
Real‐time imaging of density ducts between the plasmasphere and ionosphere
FOREGROUNDS IN WIDE-FIELD REDSHIFTED 21 cm POWER SPECTRA
UWA Profiles and Research Repository (University of Western Australia) 2015cited by 84position: middle
The High Time and Frequency Resolution Capabilities of the Murchison Widefield Array
Measuring phased‐array antenna beampatterns with high dynamic range for the Murchison Widefield Array using 137 MHz ORBCOMM satellites
A SEARCH FOR FAST RADIO BURSTS AT LOW FREQUENCIES WITH MURCHISON WIDEFIELD ARRAY HIGH TIME RESOLUTION IMAGING
wsclean: an implementation of a fast, generic wide-field imager for radio astronomy
Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data
Modelling of the spectral energy distribution of Fornax A: leptonic and hadronic production of high-energy emission from the radio lobes
Limits on low-frequency radio emission from southern exoplanets with the Murchison Widefield Array
The Murchison Widefield Array: The Square Kilometre Array Precursor at Low Radio Frequencies
Science with the Murchison Widefield Array