Topological data analysis (TDA) can broadly be described as a collection of data analysis
methods that find structure in data. These methods include clustering, manifold estimation …

This work investigates the alignment of galactic spins with the cosmic web across cosmic
time using the cosmological hydrodynamical simulation Horizon-AGN. The cosmic web …

We use a mass complete (log ($ M/{M} _ {\odot} $) $\geqslant\, 9.6$) sample of galaxies with
accurate photometric redshifts in the COSMOS field to construct the density field and the …

Galaxy formation theories predict that galaxy shapes and angular momenta have
nonrandom alignments with the cosmic web. This leads to so-called intrinsic alignment …

We study the effects of filaments on galaxy properties in the Sloan Digital Sky Survey
(SDSS) Data Release 12 using filaments from the 'Cosmic Web Reconstruction'catalogue, a …

The Cosmic Web is a complex network of filaments, walls, and voids that represent the
largest structures in the Universe. In this network, which is the direct result of structure …

Context. The interstellar medium is observed to be organized in filamentary structures, and
in neutral (HI) and ionized (H II) bubbles. The expanding nature of these bubbles shapes the …

Filaments and clusters of the cosmic web have an impact on the properties of galaxies. They
switch off their star-formation, contribute to the build-up of their stellar mass, and affect the …

In this paper, we exploit a large suite of enzo cosmological magneto-hydrodynamical
simulations adopting uniform mesh resolution, to investigate the properties of cosmic …

Intrinsic galaxy shape and angular momentum alignments can arise in cosmological large-
scale structure due to tidal interactions or galaxy formation processes. Cosmological …