  We present in this paper the analysis of the measurement of the unknown PMNS
parameters $\theta_{13}$ and $\delta$ at future LBL facilities performing
complete three parameters fits, each time fully including in the fit one of the
atmospheric and solar oscillation parameters within its present (future) error.
We show that, due to the presence of degeneracies, present uncertainties on
$\theta_{23}$ and $\Delta m^2_{23}$ worsen significantly the precision on
($\theta_{13}$,$\delta$) at future LBL experiments. Only if a precision on the
atmospheric parameters at least similar to what expected at T2K-I is reached,
then the sensitivities to $\theta_{13}$ and $\delta$ that have been presented
in the literature for many facilities (where $\theta_{23}$ and $\Delta
m^2_{23}$ are generally considered as fixed external inputs) can indeed be
almost recovered.On the other hand, the impact on this measurement of the
uncertainties on the solar parameters, $\theta_{12}$ and $\Delta m^2_{12}$ is
already negligible. Our analysis has been performed using three reference
setups: the SPL Super-Beam and the standard low-$\gamma$ $\beta$-Beam, both
aiming toward a Mton Water \v{C}erenkov detector located at L=130 km; the 50
GeV Neutrino Factory with a 40 kton Magnetized Iron Detector to look for the
``golden channel'' $\nu_e \to \nu_\mu$ with baseline L=3000 km and a 4 kton
Emulsion Cloud Chamber to look for the ``silver channel'' $\nu_e \to \nu_\tau$
with baseline L=732 km.
