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Martin Meyer is an Associate Professor at the University of Western Australia with a focus on astronomy, specifically in the field of extragalactic astronomy and galaxy evolution. His research primarily investigates the role of neutral atomic hydrogen (HI) in the formation and evolution of galaxies. He leads the DINGO survey, which conducts deep HI observations using the Australian SKA Pathfinder to understand the HI content of the Universe over the past 4 billion years. Additionally, he is involved in the CHILES project, a deep HI survey conducted with the Very Large Array, and co-chairs the SKA HI galaxy science working group. His expertise encompasses various research areas within astronomy, including galaxy morphology and interactions.
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