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 …

The IllustrisTNG project is a new suite of cosmological magnetohydrodynamical simulations
of galaxy formation performed with the arepo code and updated models for feedback …

Intracluster light (ICL) is diffuse light from stars that are gravitationally bound not to individual
member galaxies, but to the halo of galaxy clusters. Leading theories, predict that the ICL …

We investigate the formation of brightest cluster galaxies (BCGs) in the TNG300
cosmological simulation of the IllustrisTNG project. Our cluster sample consists of 700 …

Using MUSE observations from the GASP survey, we study 54 galaxies undergoing ram
pressure stripping (RPS) and spanning a wide range in galaxy mass and host cluster mass …

The bulk of stars in galaxy clusters are confined within their constituent galaxies. Those stars
do not trace the extended distribution of dark matter well as they are located in the central …

Using data collected by the Dark Energy Survey (DES), we report the detection of
intracluster light (ICL) with∼ 300 galaxy clusters in the redshift range of 0.2–0.3. We design …

The ubiquitous presence of Galactic cirri in deep optical images represents a major obstacle
to study the low surface brightness features of extragalactic sources. To address this issue …

We estimate the intracluster light (ICL) component within a sample of 18 clusters detected in
the XMM Cluster Survey (XCS) data using the deep (∼ 26.8 mag) Hyper Suprime-Cam …