"Astrophysics - Cosmology and Nongalactic Astrophysics"

Cosmological model parameter dependence of the matter power spectrum covariance from the DEUS-PUR Cosmo simulations

Future galaxy surveys will provide accurate measurements of the matter power spectrum across an unprecedented range of scales and redshifts. The analysis of these data will require one to accurately model the imprint of non-linearities of the matter …

Euclid: Reconstruction of weak-lensing mass maps for non-Gaussianity studies

Weak lensing, which is the deflection of light by matter along the line of sight, has proven to be an efficient method for constraining models of structure formation and reveal the nature of dark energy. So far, most weak-lensing studies have focused …