My research focuses on creating high performance simulations of cosmic flows and on understanding the origin of cosmic objects such as stars and galaxies. I am the main developer of the RAMSES code, a massively parallel Adaptive Mesh Refinement code for self-gravitating, magnetized, radiative flows. Together with my colleagues we are playing a very central role in the preparation and the anticipated data analysis of Euclid. I am coordinating the Cosmological Simulation Working Group of the Euclid Consortium.
The full list of the students that I am working with can be found here http://www.ics.uzh.ch/~teyssier/people.html.