  Flat spectrum radio quasars (FSRQs) are a particular class of blazars rich of
optical/ultraviolet photons inside the broad line region (BLR), necessarily
implying a huge optical depth for $\gamma$ rays above 20 GeV. As a consequence,
photons with energy above such a threshold should not be emitted. However,
photons in the energy range 70 - 400 GeV have been observed by MAGIC from the
FSRQ PKS 1222+216. Several astrophysical explanations exist in the literature,
but they are all ad hoc, namely devised only for that specific purpose. We show
that such a surprising discovery can be explained within standard blazar models
by adding the new possibility that photons oscillate into axion-like particles
(ALPs) and vice-versa inside the source. Through the photon-ALP oscillation
mechanism a sizable fraction of very-high energy (VHE) photons can escape
absorption from the BLR in a similar fashion as they largely avoid absorption
from the extragalactic background light (EBL) in the intergalactic space.
Actually, we show that not only are VHE photon indeed emitted, but also that
their spectral energy distribution (SED) is such that they lie on the same
Compton peak to which also lower energy photons simultaneously detected by
Fermi/LAT belong.
