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In this paper we calculate the energy distribution of the Mu-in Park, Kehagias-Sfetsos (KS) and L"u, Mei and Pope (LMP) black holes in the Ho\v{r}ava-Lifshitz theory of gravity. These black hole solutions correspond to the standard Einstein-Hilbert action in the infrared limit. For our calculations we use the Einstein and M{\o}ller prescriptions. Various limiting and particular cases are also discussed.

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