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Radio galaxies can extend far beyond the stellar component of their originating host galaxies, and their radio emission can consist of multiple discrete components. Furthermore, the apparent source st...

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

The broad-band radio spectral energy distribution (SED) of star-forming galaxies (SFGs) contains a wealth of complex physics. We aim to determine the physical emission and loss processes causing radio...