We review current understanding of the population of radio galaxies and radio-loud quasars
from an observational perspective, focusing on their large-scale structures and dynamics …

We explore the kinematics of 27 z≳ 6 quasar host galaxies observed in [C ii] 158 μm ([C ii])
emission with the Atacama Large Millimeter/submillimeter Array at a resolution of≈ 025. We …

Spiral galaxies have distinct internal structures, including a stellar bulge, a disk, and spiral
arms. It is unknown when in cosmic history these structures formed. In this study, we …

Massive starburst galaxies in the early Universe are estimated to have depletion times of∼
100 Myr and thus be able to convert their gas very quickly into stars, possibly leading to a …

Quenched galaxies are often observed to contain a strong bulge component. The key
question is whether this reflects a causal connection–can star formation be quenched …

We present a CO dynamical estimate of the mass of the supermassive black hole (SMBH) in
three nearby early-type galaxies: NGC 0612, NGC 1574, and NGC 4261. Our analysis is …

We use high-resolution maps of the molecular interstellar medium (ISM) in the centres of 86
nearby galaxies from the millimetre-Wave Interferometric Survey of Dark Object Masses …

Feedback from low-excitation radio galaxies (LERGs) plays a key role in the lifecycle of
massive galaxies in the local Universe; their evolution, and the impact of these active …

We present a study of the molecular gas of seven early-type galaxies with high angular
resolution data obtained as part of the mm-Wave Interferometric Survey of Dark Object …

Abstract We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 5 and
Cycle 6 observations of CO (2− 1) and CO (3− 2) emission at 0 farcs 2− 0 farcs 3 resolution …