Compact steep-spectrum (CSS) and peaked-spectrum (PS) radio sources are compact,
powerful radio sources. The multi-frequency observational properties and current theories …

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 …

Abstract The Very Large Array Sky Survey (VLASS) is a synoptic, all-sky radio sky survey
with a unique combination of high angular resolution (≈ 2 farcs 5), sensitivity (a 1σ goal of …

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 …

We have performed a search over 3440 deg 2 of Epoch 1 (2017–2019) of the Very Large
Array Sky Survey to identify unobscured quasars in the optical (0.2< z< 3.2) and obscured …

We cross-correlate the largest available mid-infrared (Wide-field Infrared Survey Explorer–
WISE), X-ray (3XMM) and radio (Faint Images of the Radio Sky at Twenty centimetres+ …

We study stellar and black hole mass assembly in a sample of 42 infrared-luminous galaxy
mergers at z< 0.3 by combining results from radiative transfer modelling with archival …

We present ALMA observations of cold dust and molecular gas in four high-luminosity,
heavily reddened (AV∼ 2.5–6 mag) type 1 quasars at z∼ 2.5 with virial M BH∼ 1010 M⊙ …

We present ALMA Band 7 observations at m of 20 luminous ([erg s− 1]) unobscured quasars
at z∼ 2. We detect continuum emission for 19/20 quasars. After subtracting an AGN …

We present the ultraviolet to submillimetre spectral energy distributions (SEDs) of the
HERschel Ultra Luminous Infrared Galaxy Survey (HERUS) sample of 42 local …