  Properties of Schroedinger black holes are derived from AdS black holes
expressed in light-cone coordinates with a particular normalization. The
advantages of this method over the direct analysis of the Schroedinger geometry
are the simplicity and the well-defined Brown-York procedure with the standard
counterterms. The method is demonstrated for several physical interests,
including the computation of the DC conductivity and the derivation of the
R-charged black hole thermodynamic properties.
