Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …

Astronomy, being one of the oldest observational sciences, has collected a lot of data over
the ages. In recent times, it is experiencing a huge data surge due to advancements in …

We introduce an updated physical model to simulate the formation and evolution of galaxies
in cosmological, large-scale gravity+ magnetohydrodynamical simulations with the moving …

We present the final sample of the Exploration of Local VolumE Satellites (ELVES) survey, a
survey of the dwarf satellites of a nearly volume-limited sample of Milky Way (MW)− like …

Abstract We present the Canada–France–Hawaii Telescope Lensing Survey (CFHTLenS)
that accurately determines a weak gravitational lensing signal from the full 154 deg2 of deep …

We study the volume-limited and nearly mass-selected (stellar mass M stars≳ 6× 109 M⊙)
ATLAS3D sample of 260 early-type galaxies (ETGs, ellipticals Es and lenticulars S0s). We …

In the companion Paper XV of this series, we derive accurate total mass-to-light ratios within
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …

Abstract We introduce the MOdelling Star cluster population Assembly In Cosmological
Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models …

We present an end-to-end, two-phase model for the origin of globular clusters (GCs). In the
model, populations of stellar clusters form in the high-pressure discs of high-redshift (z> 2) …

We report the discovery of 854 ultra-diffuse galaxies (UDGs) in the Coma cluster using deep
R band images, with partial B, i, and Hα band coverage, obtained with the Subaru telescope …