We are a theoretical cosmology group especially interested in the late-time universe. The overall aim of our research is to learn how effects of general relativity and structures, from individual particles to large-scale cosmological structures, impact the evolution of the Universe and cosmological observations. Besides considering traditional observables such as redshift-distance relations, we are focused on real-time cosmology such as redshift drift.
Our work requires analytical derivations but the main part of our work is numerical. Our work is often based on making models of the Universe and synthetic observations in these. The models that we make can either be based on exact solutions to Einstein's field equations, simple toy-models or state-of-the art simulations.
