The wealth of incoming and future cosmological observations will allow us to map out the
structure and evolution of the observable universe to an unprecedented level of precision …

The alignments between galaxies, their underlying matter structures, and the cosmic web
constitute vital ingredients for a comprehensive understanding of gravity, the nature of …

We study the angular-momentum (AM) buildup in high-z massive galaxies using high-
resolution cosmological simulations. The AM originates in co-planar streams of cold gas and …

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

On very large scales, density fluctuations in the Universe are small, suggesting a
perturbative model for large-scale clustering of galaxies (or other dark matter tracers), in …

Using a series of high-resolution N-body simulations of the concordance cosmology we
investigate how the formation histories, shapes and angular momenta of dark matter haloes …

We investigate the spins and shapes of over a million dark matter haloes identified at z= 0 in
the Millennium simulation. Our sample spans halo masses ranging from dwarf galaxies to …

The major morphological features of a galaxy are thought to be determined by the assembly
history and net spin of its surrounding dark halo. In the simplest scenario, disc galaxies form …

We investigate the alignment of the spin of dark matter haloes relative (i) to the surrounding
large-scale filamentary structure, and (ii) to the tidal tensor eigenvectors using the Horizon …

We investigate how the shapes and angular momenta of galaxy and group mass dark matter
halos in a ΛCDM N-body simulation are correlated internally and how they are aligned with …