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 …

We present cosmology results from a blinded joint analysis of cosmic shear, ξ±(ϑ), galaxy-
galaxy weak lensing, Δ Σ (R), and projected galaxy clustering, wp (R), measured from the …

Luminous red galaxies (LRGs) and blue star-forming emission-line galaxies (ELGs) are key
tracers of large-scale structure used by cosmological surveys. Theoretical predictions for …

We present the results obtained from the full-shape cosmology analysis of the redshift-space
power spectra for four galaxy samples of the SDSS-III BOSS DR12 galaxy catalog over 0.2< …

Approximate methods to populate dark-matter haloes with galaxies are of great utility to
galaxy surveys. However, the limitations of simple halo occupation models (HODs) preclude …

We present high-fidelity cosmology results from a blinded joint analysis of galaxy-galaxy
weak lensing (Δ Σ) and projected galaxy clustering (wp) measured from the Hyper Suprime …

We introduce a novel technique for constraining cosmological parameters and galaxy
assembly bias using non-linear redshift-space clustering of galaxies. We scale cosmological …

Understanding the galaxy-halo connection is fundamental for contemporary models of
galaxy clustering. The extent to which the haloes' assembly history and environment impact …

Building accurate and flexible galaxy–halo connection models is crucial in modelling galaxy
clustering on non-linear scales. Recent studies have found that halo concentration by itself …

The spatial distribution of galaxies and their gravitational lensing signal offer complementary
tests of galaxy formation physics and cosmology. However, their synergy can only be fully …