  We discuss the information loss issue for completely evaporating black holes
in the context of a globally hyperbolic spacetime that maintains unchanged the
entire semiclassical picture except for the ``last evaporation breath,'' which
pertains to full quantum gravity. Even though observers outside the black hole
cannot access information that enters the horizon, there is no actual loss of
information since it is carried over from one Cauchy surface to the next
(provided the evolution is unitary).
