Area of research
Astronomy and Astrophysics · Aerospace Engineering
Research interest
Research interests include Radio Astronomy Observations and Technology, Astrophysics and Cosmic Phenomena, Antenna Design and Optimization, and Radio Wave Propagation Studies.
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
Optimizing sparse RFI prediction using deep learning
Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWA
The impact of modelling errors on interferometer calibration for 21 cm power spectra
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 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 HYDROGEN EPOCH OF REIONIZATION ARRAY DISH. I. BEAM PATTERN MEASUREMENTS AND SCIENCE IMPLICATIONS
Constraining high-redshift X-ray sources with next generation 21-cm power spectrum measurements
Brute-force mapmaking with compact interferometers: a MITEoR northern sky map from 128 to 175 MHz
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
MITEoR: a scalable interferometer for precision 21 cm cosmology
Reionization and beyond: detecting the peaks of the cosmological 21 cm signal
Modelling of the spectral energy distribution of Fornax A: leptonic and hadronic production of high-energy emission from the radio lobes
ON THE DETECTION AND TRACKING OF SPACE DEBRIS USING THE MURCHISON WIDEFIELD ARRAY. I. SIMULATIONS AND TEST OBSERVATIONS DEMONSTRATE FEASIBILITY
An Overview of the SPTpol Experiment
Optical and Thermal Properties of ANL/KICP Polarization Sensitive Bolometers for SPTpol