  We investigate the superfluid properties of the inner crust of neutron stars
at finite temperature for different pairing functionals. We generalize the
formalism adopted in previous article to include the effect of the temperature
to calculate the specific heat of each given Wigner-Seitz cell. The
calculations are done for two pairing forces, Gogny D1 and $V_{\text{low-k}}$,
with finite range and a density dependent contact interaction. We compare in
such a way the effect of the pairing strength and of the range on the thermal
properties of the inner crust.
