Through developing semi-analytic models and using state-of-the-art cosmological hydrodynamic simulations, my research focusses on the formation and evolution of galaxies. Principally, I am currently working with the IllustrisTNG simulations, processing them to understand the atomic and molecular gas content of galaxies. I am also the lead developer of the DARK SAGE semi-analytic model of galaxy formation and a member of the WALLABY H I survey team.
For more information, please see my personal website.
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