  Misaligned AGN (MAGNs), i.e., radio-loud AGNs with the jet not pointing
directly towards us, represent a new class of GeV emitters revealed by the
Fermi space telescope. Although they comprise only a small fraction of the
high-energy sources, MAGNs are extremely interesting objects offering a
different perspective to study high-energy processes with respect to blazars.
The aim of this work is to evaluate the impact of the new-generation Cherenkov
Telescope Array (CTA) on the MAGN class and propose possible observational
strategies to optimize their detection.
