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 …

The cosmic web is the largest scale manifestation of the anisotropic gravitational collapse of
matter. It represents the transitional stage between linear and non-linear structures and …

The cosmic web is one of the most striking features of the distribution of galaxies and dark
matter on the largest scales in the Universe. It is composed of dense regions packed full of …

The role of the cosmic web in sha** galaxy properties is investigated in the Galaxy And
Mass Assembly (GAMA) spectroscopic survey in the redshift range 0.03≤ z≤ 0.25. The …

The main feature of the spatial large-scale galaxy distribution is its intricate network of
galaxy filaments. This network is spanned by the galaxy locations that can be interpreted as …

Abstract zobov (ZOnes Bordering On Voidness) is an algorithm that finds density
depressions in a set of points, without any free parameters, or assumptions about shape. It …

We analyse the structure and connectivity of the distinct morphologies that define the cosmic
web. With the help of our multiscale morphology filter (MMF), we dissect the matter …

We introduce the NEXUS algorithm for the identification of cosmic web environments:
clusters, filaments, walls and voids. This is a multiscale and automatic morphological …

In this paper, we propose a new dynamical classification of the cosmic web. Each point in
space is classified in one of four possible web types: voids, sheets, filaments and knots. The …

The variation of galaxy stellar masses and colour types with the distance to projected cosmic
filaments are quantified using the precise photometric redshifts of the COSMOS2015 …