We review the properties and nature of luminous high-redshift radio galaxies (HzRGs, z> 2)
and the environments in which they are located. HzRGs have several distinct constituents …

The emergence of the first sources of light at redshifts of z∼ 10–30 signaled the transition
from the simple initial state of the Universe to one of increasing complexity. Recent progress …

The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a
telescope under development by a consortium of 17 countries. The SKA will be 50 times …

EMU is a wide-field radio continuum survey planned for the new Australian Square
Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep …

Quasar feedback in the form of powerful outflows is invoked as a key mechanism to quench
star formation in galaxies, preventing massive galaxies to overgrow and producing the red …

Pressure-regulated star formation is a simple variant on the usual supernova-regulated star
formation efficiency that controls the global star formation rate as a function of cold gas …

We examine the detailed physics of the feedback mechanism by relativistic active galactic
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …

Feedback from active galactic nuclei (AGN) has become a major component in simulations
of galaxy evolution, in particular for massive galaxies. AGN jets have been shown to provide …

Context. Sources at the brightest end of the quasi-stellar object (QSO) luminosity function,
during the peak epoch in the history of star formation and black hole accretion (z∼ 2− 4 …

We apply a turbulence-regulated model of star formation to calculate the star formation rate
(SFR) of dense star-forming clouds in simulations of jet–interstellar medium (ISM) …