  We study the entropy-corrected version of the new agegraphic dark energy
(NADE) model and dark matter in a spatially non-flat Universe and in the
framework of Ho\v{r}ava-Lifshitz cosmology. For the two cases containing
noninteracting and interacting entropy-corrected NADE (ECNADE) models, we
derive the exact differential equation that determines the evolution of the
ECNADE density parameter. Also the deceleration parameter is obtained.
Furthermore, using a parametrization of the equation of state parameter of the
ECNADE model as $\omega_{\Lambda}(z)=\omega_0+\omega_1 z$, we obtain both
$\omega_0$ and $\omega_1$. We find that in the presence of interaction, the
equation of state parameter $\omega_0$ of this model can cross the phantom
divide line which is compatible with the observation.
