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As mentioned in the previous section, at low redshift Faraday rotation does not depend on ra- dio source morphology or luminosity: this might not be the case at high redshift, where
We started 607-MHz GMRT observation of these can- didate DDRGs to image the different components, estimate the flux densities and spectral indices of the outer and inner lobes in order
Having established that the cluster association fraction is related to radio luminosity, we next investigated whether the mean rich- ness of the associated clusters is related to
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Since a few of the core prominences of our active sources are comparable to that of the upper limits on the candidate remnants, our results demonstrate that radio-loud AGN with
At LOFAR frequencies it was possible to resolve the inner structure of the radio emission of the galaxy group MaxBCG J199, hosting a central radio galaxy which shows opposing
Our main observational conclusions are: (i) in line with previous studies, the dust detection rate is higher in radio-jet galaxies than in non radio-jet galaxies; (ii) radio