This overview paper describes the legacy prospect and discovery potential of the Dark
Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the …

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 …

We introduce the Hydrangea simulations, a suite of 24 cosmological hydrodynamic zoom-in
simulations of massive galaxy clusters (M 200c= 1014–1015.4 M⊙) with baryon particle …

We study the effects of the local environment and stellar mass on galaxy properties using a
mass complete sample of quiescent and star-forming systems in the COSMOS field at …

Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …

We report the first results from the Clusters Around Radio-Loud AGN program, a Cycle 7 and
8 Spitzer Space Telescope snapshot program to investigate the environments of a large …

Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

Multi-phase filamentary structures around brightest cluster galaxies (BCG) are likely a key
step of AGN-feedback. We observed molecular gas in three cool cluster cores, namely …

We present photometric redshift estimates for galaxies used in the weak lensing analysis of
the Dark Energy Survey Science Verification (DES SV) data. Four model-or machine …

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