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

Superfluid properties of the inner crust of neutron stars. II. Wigner-Seitz cells at finite temperature