Active galactic nuclei (AGN) are energetic astrophysical sources powered by accretion onto
supermassive black holes in galaxies, and present unique observational signatures that …

Active galactic nuclei (AGN) are powered by the accretion of material onto a supermassive
black hole (SMBH) and are among the most luminous objects in the Universe. However, the …

We present integral field unit observations covering the [o iii] λλ4959, 5007 and Hβ emission
lines of 16 z< 0.2 type 2 active galactic nuclei (AGN). Our targets are selected from a well …

ABSTRACT A two-parameter semi-empirical model is presented for the spectral energy
distributions of galaxies with contributions to their infrared–submillimeter–radio emission …

Over the past decade, several works have used the ratio between total (rest 8− 1000 μm)
infrared and radio (rest 1.4 GHz) luminosity in star-forming galaxies (q IR), often referred to …

We review results from cosmic X-ray surveys of active galactic nuclei (AGNs) over the past
≈ 15≈ 15 years that have dramatically improved our understanding of growing …

Abstract We present 1–7 GHz high-resolution radio imaging (VLA and e-MERLIN) and
spatially resolved ionized gas kinematics for 10 z< 0.2 type 2 'obscured'quasars (log [L …

We examine the behaviour of the infrared-radio correlation (IRRC) over the range 0< z≲ 6
using new, highly sensitive 3 GHz observations with the Karl G. Jansky Very Large Array …

We use deep panchromatic data sets in the GOODS-N field, from GALEX to the deepest
Herschel far-infrared (FIR) and VLA radio continuum imaging, to explore the evolution of star …

We explore the multiwavelength properties of AGN host galaxies for different classes of
radio-selected AGN out to z≲ 6 via a multiwavelength analysis of about 7700 radio sources …