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 …

Abstract We present Atacama Large Millimeter Array 1 mm observations of the rest-frame far-
infrared (FIR) dust continuum in 27 quasars at redshifts 6.0≲ z< 6.7. We detect FIR emission …

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 …

We investigate the mean star formation rates (SFRs) in the host galaxies of∼ 3000 optically
selected quasi-stellar objects (QSOs) from the Sloan Digital Sky Survey within the Herschel …

Accurate active galactic nucleus (AGN) identifications and spatially resolved host galaxy
properties are a powerful combination for studies of the role of AGNs and AGN feedback in …

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 …

What determines the nuclear radio emission in local galaxies? To address this question, we
combine optical [O iii] line emission, robust black hole (BH) mass estimates, and high …

We have observed 104 gravitationally lensed quasars at z∼ 1–4 with Herschel/SPIRE, the
largest such sample ever studied. By targeting gravitational lenses, we probe intrinsic far …

In order to understand the role of radio-quiet quasars (RQQs) in galaxy evolution, we must
determine the relative levels of accretion and star-formation activity within these objects …

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 …