  We study tunneling of massless and massive particles through the smeared
quantum horizon of the extra-dimensional Schwarzschild black holes. The
emission rate of the particles' tunneling is modified by noncommutativity
effects in a bulk spacetime of dimension $d$. The issues of information loss
and possible correlations between emitted particles are discussed. We show that
even by considering both noncommutativity and braneworld effects, there is no
correlation between different modes of evaporation at least at late-time and
within approximations used in the calculations. However, incorporation of
quantum gravity effects such as modification of the standard dispersion
relation or generalization of the Heisenberg uncertainty principle, leads to
the correlation between emitted particles. Although time-evolution of these
correlations is not trivial, a part of information coming out of the black hole
can be preserved in these correlations. On the other hand, as a well-known
result of spacetime noncommutativity, a part of information may be preserved in
a stable black hole remnant.
