  IceCube has observed an excess of neutrino events over expectations from the
isotropic background from the direction of NGC 1068. The excess is inconsistent
with background expectations at the level of $2.9\sigma$ after accounting for
statistical trials. Even though the excess is not statistical significant yet,
it is interesting to entertain the possibility that it corresponds to a real
signal. Assuming a single power-law spectrum, the IceCube Collaboration has
reported a best-fit flux $\phi_\nu\sim 3 \times 10^{-8} (E_\nu/{\rm
TeV})^{-3.2}~({\rm GeV \, cm^2 \, s})^{-1}$, where $E_\nu$ is the neutrino
energy. Taking account of new physics and astronomy developments we give a
revised high-energy neutrino flux for the Stecker-Done-Salamon-Sommers AGN core
model and show that it can accommodate IceCube observations.
