  Starting from a complete sample of type I AGN observed by INTEGRAL in the
20-40 keV band, we have selected a set of 8 AGN which can be classified as
radio loud objects according to their 1.4 GHz power density, radio to hard
X-ray flux flux density ratio and radio morphology. The sample contains 6 Broad
Line Radio Galaxies and 2 candidate ones. Most of the objects in our sample
display a double lobe morphology, both on small and large scales. For all the
objects, we present broad-band (1-110 keV) spectral analysis using INTEGRAL
observations together with archival XMM-Newton, Chandra, Swift/XRT and
Swift/BAT data. We constrain the primary continuum (photon index and cut-off
energy), intrinsic absorption and reprocessing features (iron line and
reflection) in most of the objects. The sources analysed here show remarkable
similarities to radio quiet type 1 AGN with respect to most of the parameters
analysed; we only find marginal evidence for weaker reprocessing features in
our objects compared to their radio quiet counterparts. Similarly we do not
find any correlation between the spectral parameters studied and the source
core dominance or radio to 20-100 keV flux density ratios, suggesting that what
makes our objects radio loud has no effect on their high energy
characteristics.
