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 present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, 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 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 …

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 …

Present-day clusters are massive halos containing mostly quiescent galaxies, while distant
protoclusters are extended structures containing numerous star-forming galaxies. We …

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 …

We have obtained three-dimensional maps of the universe in∼ 200× 200× 80 comoving
Mpc 3 (cMpc 3) volumes each at z= 5.7 and 6.6 based on a spectroscopic sample of 179 …

Faint star-forming galaxies at z∼ 2–3 can be used as alternative background sources to
probe the Lyα forest in addition to quasars, yielding high sightline densities that enable 3D …