The Group
Our mutli-disciplinary group combines theoretical and numerical radiation-hydrodynamics methods with the unprecedented data provided by the new MUSE integral-field-spectrograph on the ESO/Very-Large-Telescope to advance our knowledge on the physics of the Intergalactic and Circumgalactic media. The group was established in 2016 as a part of the Swiss National Science Foundation Professorship Grant: "From Cosmic Web to Galaxies: illuminating the gaseous link between the Dark and the Bright Universe" (PI: S. Cantalupo) and include PhD student and postdoctoral members (G. Pezzulli, A.-C. Vossberg) working in close collaboration with other members of the MUSE consortium at ETH (S. Gallego, R. Marino, from Lilly's group).