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Radio-Loud (RL) Active Galactic Nuclei (AGNs) are among the brightestastrophysical sources at all wavelengths. Their relativistic jets can affectboth their Supermassive Black Holes (SMBHs) growth and the surroundingintergalactic medium. While in the radio band these jets can be observed at allscales (from pc to Mpc scales), their X-ray and {\gamma}-ray emission isexpected to be concentrated on very small scales (<10 pc). However, after thelaunch of the Chandra X-ray telescope, several kpc-scale jets were detected andthe mechanism responsible for their high-energy radiation at these scales isstill under debate. Understanding its origin is crucial also to derive thephysical properties of these jets (e.g. the power) at large scales and, as aconsequence, their impact on the environment. In the following, we explore theInverse Compton interaction of the relativistic electrons within relativisticjets with the Cosmic Microwave background photons (IC/CMB) as possibleinterpretation. Moreover, we also estimate how this interpretation could alsoaffect the observed evolution across cosmic times of the SMBHs hosted in jettedsystems.

Impact of the CMB on the evolution of AGNs and their relativisitc jets at the highest redshift