We present an updated version of the hmcode augmented halo model that can be used to
make accurate predictions of the non-linear matter power spectrum over a wide range of …

We perform a combined analysis of cosmic shear tomography, galaxy–galaxy lensing
tomography, and redshift-space multipole power spectra (monopole and quadrupole) using …

We present an optimized variant of the halo model, designed to produce accurate matter
power spectra well into the non-linear regime for a wide range of cosmological models. To …

We present a new, updated version of the EuclidEmulator (called EuclidEmulator2), a fast
and accurate predictor for the nonlinear correction of the matter power spectrum. 2 per cent …

Current and upcoming radio telescopes will map the spatial distribution of cosmic neutral
hydrogen (H i) through its 21 cm emission. In order to extract the maximum information from …

We present an accurate non-linear matter power spectrum prediction scheme for a variety of
extensions to the standard cosmological paradigm, which uses the tuned halo model …

We test extensions to the standard cosmological model with weak gravitational lensing
tomography using 450 deg2 of imaging data from the Kilo Degree Survey (KiDS). In these …

We analyse the clustering features of Large Scale Structures (LSS) in the presence of
massive neutrinos, employing a set of large-volume, high-resolution cosmological N-body …

Gravitational weak lensing by dark matter haloes leads to a measurable imprint in the shear
correlation function of galaxies. Fuzzy dark matter (FDM), composed of ultralight axion-like …

We study the characteristics of the galaxy cluster samples expected from the European
Space Agency's Euclid satellite and forecast constraints on parameters describing a variety …