We review the field of collisionless numerical simulations for the large-scale structure of the
Universe. We start by providing the main set of equations solved by these simulations and …

This work and its companion paper, Amon et al.[Phys. Rev. D 105, 023514 (2022) PRVDAQ
2470-0010 10.1103/PhysRevD. 105.023514], present cosmic shear measurements and …

We study the cosmological information content of the redshift-space galaxy bispectrum
monopole at one-loop order in perturbation theory. We incorporate all effects necessary for …

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 …

We study the information content of the angle-averaged redshift space galaxy bispectrum.
The main novelty of our approach is the use of a systematic tree-level perturbation theory …

The current standard model of cosmology successfully describes a variety of measurements,
but the nature of its main ingredients, dark matter and dark energy, remains unknown. is a …

Since the discovery of the accelerated expansion of the present universe, significant
theoretical developments have been made in the area of modified gravity. In the meantime …

In this work, which is the first of a series to prepare a cosmological parameter analysis with
third-order cosmic shear statistics, we model both the shear three-point correlation functions …

Aims. In this work, we perform the first cosmological parameter analysis of the fourth release
of Kilo Degree Survey (KiDS-1000) data with second-and third-order shear statistics. This …

We present high signal-to-noise measurements of three-point shear correlations and the
third moment of the mass aperture statistic using the first 3 years of data from the Dark …