Warrick’s current research focus is implementing methods to match models to data that will be produced by ESA’s PLATO space observatory. He has already worked extensively on the problem of fitting stellar models to asteroseismic data and is known in particular for his work on mitigating the known biases caused by improper modelling near the stellar surface.
Before he was involved in asteroseismology, Warrick worked on modelling exotic objects known as “quasi-stars”: black holes embedded in and accreting from giant-like envelopes of gas. Along the way, he undertook some highly theoretical work on why stars evolve into red giants.