Although first considered as too diluted for the formation of molecules in-situ and too harsh
an environment for their survival, the interstellar medium has turned out to host a rich palette …

There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …

We report on the host properties of five X-ray-luminous active galactic nuclei (AGN)
identified at 3< z< 5 in the first epoch of imaging from the Cosmic Evolution Early Release …

The relationship between quasars and their host galaxies provides clues on how
supermassive black holes (SMBHs) and massive galaxies are jointly assembled. To …

Recent studies have suggested that red quasars are a phase in quasar evolution when
feedback from black hole accretion evacuates obscuring gas from the nucleus of the host …

We investigate the star-forming main sequence of the host galaxies of a large, well-defined
sample of 453 redshift∼ 0.3 quasars with previously available star formation rates by …

Dusty star-forming galaxies (DSFGs) at redshift z≥ 1 are among the most vigorously star-
forming galaxies in the Universe. However, their dense (≥ 10 5 cm− 3) gas phase–typically …

We investigate the physical properties, such as star-forming activity, disc versus bulge
nature, galaxy size, and obscuration of 3811 SRG/eROSITA-detected AGNs at 0.2< z< 0.8 in …

We present detailed and comprehensive data reduction and point-spread-function (PSF)
model construction for all public JWST NIRCam imaging data from the COSMOS-Web …

We present the discovery of a gravitationally lensed dust-reddened QSO at z= 2.517,
identified in a survey for QSOs by infrared selection. Hubble Space Telescope imaging …