I lead the Epoch of Reionisation project at ICRAR, managing a small group of researchers who are using the Murchison Widefield Array to detect the early Universe neutral hydrogen signal. We are also actively contributing to the EoR and Cosmic Dawn experiment for the Square Kilometre Array project. Our research encompasses experimental design, development and testing of statistical foreground models, optimal power spectrum estimators, and study and treatment of data systematics (e.g., effects of the ionosphere). We also process MWA EoR data through our CHIPS power spectrum estimation pipeline, with the aim to detect the EoR signal at z=6.5-9.0.
The MWA EoR program is part of the ASTRO 3D Centre of Excellence.
We have a range of statistical and observational research projects available to potential students, suiting applicants who have a strong background in statistical mathematics, low-frequency radio interferometry, or astronomical software development.
Image: Example simulated brightness temperature distribution and corresponding power spectrum at the end of the Cosmic Dawn (z=14.22). Credit: Andrei Mesinger, SNS
Signal processing theory, Epoch of Reionisation, radio astronomy instrument design considerations, radio transients
Membership and professional roles:
Chief Investigator, ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)
Past President, Astronomical Society of Australia
ARC Future Fellow
Board member, Astronomy Australia Ltd
Member, National Committee for Astronomy
Member, ASCC Science Advisory Committee
Fellow, Astronomical Society of Australia
Fellow, Australian Institute of Physics
Board Member, EoR/CD Science Working Group
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