We are interested in all aspects of galaxy formation and evolution, including star formation, massive black holes, and connections with the intergalactic medium. We address these problems using a combination of analytic modeling, numerical simulation, and comparison with observations, with an emphasis on expanding our understanding of the fundamental physical processes involved and leveraging data from new astronomical facilities. See the research page for more details.

We are core members of the FIRE (Feedback In Realistic Environments) cosmological simulation project, as part of which we develop new methods to improve the predictive power of galaxy formation theories. In collaboration with Northwestern’s visualization group, we also develop the Firefly interactive visualization app for particle-based simulations.