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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 survey team.


For more information, please see my personal website.

ICRAR Statement

The content of this page is maintained by Adam Stevens, please contact them with any questions or comments on this content.