About us

We study the formation and evolution of cosmic structures across a wide range of scales through both observations and theoretical modeling, taking into account the complexities of various astrophysical processes. Our comprehensive approach enables us to develop a more accurate and realistic understanding of how stars, galaxies, and large-scale structures form and evolve than is provided by current models alone. To achieve this, we combine observations from ground- and space-based telescopes spanning the electromagnetic spectrum with state-of-the-art numerical simulations.