I joined the ICG as a Senior Research Fellow in January 2022, supported by a Royal Society URF. Before that I was a McWilliams Fellow at Carnegie Mellon University, and before that a Junior Research Fellow at St John's College, Oxford. I obtained my PhD from Stanford University in 2017. I am interested primarily in developing new tests of the standard model of cosmology (gravity and/or dark sector physics) using astrophysical objects, mainly galaxies and stars. My work ranges from pure theory, through N-body and hydrodynamical simulations to statistical data analysis. I am also interested in galaxy formation and how best to characterise the relation between galaxies and their host dark matter halos.
