Modelling the redshift distribution of Euclid’s lensed galaxies for field-level analyses

Brief description: The goal of this PhD project is to develop a new redshift sampler for weak lensing, designed to meet the accuracy requirements of field-level inference. This sampler will combine physical models of galaxy populations with flexible machine-learning techniques. The thesis will contribute to maximising the potential of Euclid's weak lensing data and advance our understanding of the formation of cosmic structures.

Details about this position can be found here. 

Fully funded by ERC StG grant OCAPi