Supermassive black holes are found at the centres of massive galaxies. During the growth of
these black holes they light up to become visible as active galactic nuclei (AGNs) and …

Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as
the main mechanism responsible for regulating star formation in active galactic nucleus …

Abstract The Chandra Deep Fields (CDFs), being a major thrust among extragalactic X-ray
surveys and complemented effectively by multiwavelength observations, have critically …

To constrain the nature and fraction of the ionized gas outflows in active galactic nuclei
(AGNs), we perform a detailed analysis on gas kinematics as manifested by the velocity …

We present the first results from the KMOS (K-band Multi-Object Spectrograph) AGN (active
galactic nuclei) Survey at High redshift (KASH z), a VLT/KMOS integral-field spectroscopic …

We map the co-eval growth of galaxies and their central supermassive black holes in detail
by measuring the incidence of active galactic nuclei (AGNs) in galaxies as a function of star …

We present results from the MOSFIRE Deep Evolution Field (MOSDEF) survey on the
identification, selection biases, and host galaxy properties of 55 X-ray, IR, and optically …

We show how the interplay between active galactic nuclei (AGNs) and merger history
determines whether a galaxy quenches star formation (SF) at high redshift. We first simulate …

Galaxy surveys have suggested that rapid and sustained decrease in the star-formation rate
(SFR),“quenching”, in massive disk galaxies is frequently related to the presence of a bar …

Aims. We present a non-parametric morphology analysis of the stellar continuum and
nebular emission lines for a sample of local galaxies. We explore the dependence of the …