Negative feedback from active galactic nuclei (AGN) is the leading mechanism for the
quenching of massive galaxies in the vast majority of modern galaxy evolution models …

We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas
mass-selected sample of 22 star-forming galaxies at z= 0.46–3.60, observed as part of the …

Dusty star-forming galaxies at high redshift (1< z< 3) represent the most intense star-forming
regions in the universe. Key aspects to these processes are the gas heating and cooling …

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 …

Context. Sources at the brightest end of the quasi-stellar object (QSO) luminosity function,
during the peak epoch in the history of star formation and black hole accretion (z∼ 2− 4 …

We present the host-galaxy molecular gas properties of a sample of 213 nearby (0.01< z<
0.05) hard-X-ray-selected active galactic nucleus (AGN) galaxies, drawn from the 70-month …

Growing supermassive black holes (Active Galactic Nuclei; AGN) release energy with the
potential to alter their host galaxies and larger-scale environment; a process named “AGN …

We use a sample of powerful z\,≈\,0.1 type 2 quasars ('obscured'; log LAGN/erg s ^-
1\,\gtrsim\,45), which host kpc-scale ionized outflows and jets, to identify possible signatures …

We resolve the host galaxies of seven gravitationally lensed quasars at redshift 1.5–2.8
using observations with the Atacama Large (sub) Millimetre Array. Using a visibility plane …

SPT0311-58 is the most massive infrared luminous system discovered so far during the
Epoch of Reionization (EoR). In this paper, we present a detailed analysis of the molecular …