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 …

Source classifications, stellar masses, and star-formation rates are presented for≈ 80 000
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …

In this paper, we present photometric redshift (photo-z) estimates for the Dark Energy
Spectroscopic Instrument (DESI) Legacy Imaging Surveys, currently the most sensitive …

We present a detailed study of the cosmic star formation history over 90 per cent of cosmic
time (0≲ z≲ 4), using deep, radio continuum observations that probe star formation activity …

We study the nature of the faint radio source population detected in the MeerKAT
International GHz Tiered Extragalactic Exploration (MIGHTEE) Early Science data in the …

The most massive galaxies in the Universe stopped forming stars due to the time-integrated
feedback from central supermassive black holes (SMBHs). However, the exact quenching …

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 …

ABSTRACT We present the Australian Square Kilometre Array Pathfinder (ASKAP)
observations of the Galaxy and Mass Assembly (GAMA)-23h field. The survey was carried …

It is well known that supermassive black holes (SMBHs) and their host galaxies co-evolve. A
manifestation of this co-evolution is the correlation that has been found between the SMBH …

We use approximately 1800 X-ray active galactic nuclei (AGN) in the eROSITA Final
Equatorial-Depth Survey (eFEDS) that span over two orders of magnitude in X-ray …