Speaker
Bianca De Caro
(INFN-Pd)
Description
Euclid experiment will allow us to derive constraints on cosmological parameters and perform model selection through cross-correlation measurements between Cosmic Microwave Background (CMB) and Large Scale Structure (LSS). In this work we focalize on the detection of the late Integrated Sachs-Wolfe effect in order to constraint relevant cosmological parameters as the dark energy parameters and sum of neutrino masses by means of a Needlet-based cross-correlation observable.
Author
Bianca De Caro
(INFN-Pd)
