  Recent work has shown that the entropy of the non-rotating BTZ black hole can
be derived from a dual conformal description at any spatial location. In this
followup it is shown that a dual conformal description exists at any spatial
location for the rotating BTZ black hole as well. As in the non-rotating case,
two copies of the central charge $c^{\pm} = 3\ell/2G$ are recovered and the
microcanonical Cardy formula yields the correct Bekenstein-Hawking entropy.
