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We review the high energy properties of Misaligned AGNs associated withgamma-ray sources detected by Fermi in 24 months of survey. Most of them arenearby emission low power radio galaxies (i.e FRIs) which probably havestructured jets. On the contrary, high power radio sources (i.e FRIIs) with GeVemission are rare. The small number of FRIIs does not seem to be related totheir higher redshifts. Assuming proportionality between the radio core fluxand the gamma-ray flux, several of them are expected to be bright enough to bedetected above 100 MeV in spite of their distance. We suggest that beaming/jetstructural differences are responsible for the detection rate discrepancyobserved between FRIs and FRIIs.

Gamma-Rays from Radio Galaxies: Fermi-Lat Observations