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 …

We use the IllustrisTNG simulations to study the demographics and properties of jellyfish
galaxies in the full cosmological context. By jellyfish galaxies, we mean satellites orbiting in …

ABSTRACT The Deep Extragalactic VIsible Legacy Survey (DEVILS) is a large
spectroscopic campaign at the Anglo-Australian Telescope (AAT) aimed at bridging the near …

ABSTRACT The Galaxy And Mass Assembly Survey (GAMA) covers five fields with highly
complete spectroscopic coverage (> 95 per cent) to intermediate depths (r< 19.8 or i< 19.0 …

We study the stellar morphological evolution of disc galaxies within clusters in the TNG50
and TNG100 runs from the IllustrisTNG simulation suite. We select satellites of masses …

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 present the first quantitative detection of large-scale filamentary structure at z≃ 0.7 in the
large cosmological volume probed by the VIMOS Public Extragalactic Redshift Survey …

We present the first detection of mass-dependent galactic spin alignments with local cosmic
filaments with> 2σ confidence using IFS kinematics. The 3D network of cosmic filaments is …

We use a mass complete (log ( MM) 9.6) sample of galaxies with accurate photometric
redshifts in the COSMOS field to construct the density field and the cosmic web to z= 1.2 …