Analytical models describing the dynamics of lobed radio sources are essential for
interpretation of the tens of millions of radio sources that will be observed by the Square …

We simulate the evolution of relativistic electrons injected into the intracluster medium by five
radio galaxies. We study the spatial transport and the emission properties of the injected …

We present here radiosed, a Bayesian inference framework tailored to modelling and
classifying broad-band radio spectral energy distributions (SEDs) using only data from …

Context. A number of observations have revealed atomic and/or molecular lines in active
galaxies hosting jets and outflows. Line widths indicate outward motions of hundreds to a …

The origin of the diffuse gamma-ray background in the range from hundreds keV to several
MeV is not known conclusively. From current models and observations it is believed that, at …

We investigate the evolution of active galactic nucleus jets on kiloparsec-scales due to their
interaction with the clumpy interstellar medium (ISM) of the host galaxy and, subsequently …

Context. The reason why some radio galaxies (RGs) grow to form so-called giant radio
galaxies (GRGs) with sizes> 700 kpc, is still unknown. Aims. In this study, we compare the …

The bright radio source, GLEAM J091734-001243 (hereafter GLEAM J0917-0012), was
previously selected as a candidate ultra-high redshift (z> 5) radio galaxy due to its compact …

The energy coupling efficiency of active galactic nucleus (AGN) outbursts is known to differ
significantly with factors including the jet kinetic power, duration of the outburst, and …