Abstract
Abstract We have carried out a systematic analysis of all the AGN brighter than 1 Jansky at 5 GHz available in the BeppoSAX public archive. Our sample includes a total of 26 Radio-Loud AGN, 10 of which are Broad Line Radio Galaxies (BLRGs), 4 Steep Spectrum Radio Quasars (SSRQs) and 12 Flat Spectrum Radio Quasars (FSRQs). Our analysis shows spectral differences (spectral slopes, column densities and reprocessed features) among the different classes of radio-loud AGN. In addition, when compared to Seyfert 1 galaxies, BLRGs appear to have weaker iron lines. Possible reasons responsible for the observed X-ray spectral differences are investigated.
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