The diffuse light that spreads through groups and clusters of galaxies is made of free-floating
stars not bound to any galaxy. This is known as the intracluster light (ICL) and holds …

Not all the light in galaxy groups and clusters comes from stars that are bound to galaxies. A
significant fraction of it constitutes the so-called intracluster or diffuse light (ICL), a low …

ABSTRACT JWST imaging of the rich galaxy cluster Abell 2744 at z= 0.308 has been used
by the UNCOVER team to construct mosaic images in the NIRCam filters. The exceptionally …

The relation between the total mass contained in the globular clusters of a galaxy and the
mass of its dark-matter halo has been found observationally to be nearly linear over five …

Intracluster light (ICL) provides an important record of the interactions galaxy clusters have
undergone. However, we are limited in our understanding by our measurement methods. To …

In this paper, we analyse the light distribution in the Hydra I cluster of galaxies to explore
their low surface brightness features, measure the intra-cluster light, and address the …

We present a post-processing catalogue of globular clusters (GCs) for the 39 most massive
groups and clusters in the TNG50 simulation of the IlllustrisTNG project (virial masses] M⊙) …

We present a survey of globular clusters (GCs) in the massive gravitational lens cluster
SMACS J0723. 3–7327 at z= 0.39 based on the early released JWST/NIRCam images. In …

The Fornax cluster provides an unparalleled opportunity of investigating the formation and
evolution of early-type galaxies in a dense environment in detail. We aim at kinematically …

The current properties of globular cluster systems (GCSs) are the result of the evolution
experienced by their host galaxies, which shape the richness of the GCS as well as its …