We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr
treasury program conducted by the James Webb Space Telescope in its first cycle of …

The study of galaxy protoclusters is beginning to fill in unknown details of the important
phase of the assembly of clusters and cluster galaxies. This review describes the current …

We report the discovery of a remarkable concentration of massive galaxies with extended X-
ray emission at z spec= 2.506, which contains 11 massive (M*≳ 10 11 M⊙) galaxies in the …

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 identification of an extreme protocluster of galaxies in the early universe
whose core (nicknamed Distant Red Core, DRC, because of its very red color in Herschel …

Galaxy clusters are the endpoints of structure formation and are continuously growing
through the merging and accretion of smaller structures. Numerical simulations predict that a …

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 …

Context. According to the current paradigm of galaxy formation, the first galaxies likely
formed within large dark matter haloes. The fragmentation of these massive haloes led to the …

Our statistical understanding of galaxy evolution is fundamentally driven by objects that lie
above the surface-brightness limits of current wide-area surveys (μ∼ 23 mag arcsec− 2) …

We study the connection between morphology and dynamical state of the simulated galaxy
clusters in z∈[0, 1.031] from The Three Hundred project. We quantify cluster dynamical state …