2007MNRAS.376..151J

We present an XMM-Newton observation of the radio galaxy 4C 23.56 at z = 2.48 which reveals extended X-ray emission coincident with the radio lobes spanning ∼0.5 Mpc. These are the largest X-ray-bright lobes known at z > 2. Under the assumption that these features result from inverse-Compton scattering of cosmic microwave background photons by relativistic electrons in the radio source lobes, the measured luminosity of L_0.5–8keV = 7.5x10⁴⁴ erg/s implies that minimum energy stored within the lobes is ∼10⁵⁹ erg. We discuss the potential of the large-scale radio/X-ray lobes to influence evolution of the host galaxy and protocluster environment at high redshift.