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We have analyzed the NVSS and SUMSS data at 1.4 GHz and 843 MHz for a welldefined complete sample of hard X-ray AGN observed by INTEGRAL. A large number(70/79) of sources are detected in the radio band, showing a wide range ofradio morphologies, from unresolved or slightly resolved cores to extendedemission over several hundreds of kpc scales. The radio fluxes have beencorrelated with the 2-10 keV and 20-100 keV emission, revealing significantcorrelations with slopes consistent with those expected for radiativelyefficient accreting systems. The high energy emission coming from the inneraccretion regions correlates with the radio emission averaged over hundreds ofkpc scales (i.e., thousands of years).

The 1.4 GHz radio properties of hard X-ray selected AGN