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, Radio Wave Propagation Studies, and Antenna Design and Optimization.
Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning
Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations
First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
HERA Phase I Limits on the Cosmic 21 cm Signal: Constraints on Astrophysics and Cosmology during the Epoch of Reionization
Mitigating Internal Instrument Coupling for 21 cm Cosmology. II. A Method Demonstration with the Hydrogen Epoch of Reionization Array
Redundant-baseline calibration of the hydrogen epoch of reionization array
Effective range of non-cell autonomous activator and inhibitor peptides specifying plant stomatal patterning
Optimizing sparse RFI prediction using deep learning
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
Low Altitude Solar Magnetic Reconnection, Type III Solar Radio Bursts, and X-ray Emissions
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 Murchison Widefield Array Commissioning Survey: A Low-Frequency Catalogue of 14 110 Compact Radio Sources over 6 100 Square Degrees
2016cited by 65position: middle
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