  In this short note, I present a generalization of a set of static
D-dimensional (D >= 3) Lifshitz black holes, which are solutions of the
gravitational model obtained by amending the cosmological Einstein theory with
the addition of only the curvature-scalar-squared term and that are described
by two parameters, to a more general class of exact, analytic solutions that
involves an additional parameter which now renders them stationary. In the
special D=3 and the dynamical exponent z=1 case, the parameters can be adjusted
so that the solution becomes identical to the celebrated BTZ black hole metric.
