  In arbitrary dimension, we consider a theory described by the most general
quadratic curvature corrections of Einstein gravity together with a
self-interacting nonminimally coupled scalar field. This theory is shown to
admit five different families of Lifshitz black holes dressed with a nontrivial
scalar field. The entropy of these configurations is microscopically computed
by means of a higher-dimensional anisotropic Cardy-like formula where the role
of the ground state is played by the soliton obtained through a double analytic
continuation. This involves to calculate the correct expressions for the masses
of the higher-dimensional Lifshitz black hole as well as their corresponding
soliton. The robustness of this Cardy-like formula is checked by showing that
the microscopic entropy is in perfect agreement with the gravitational Wald
entropy. Consequently, the calculated global charges are compatible with the
first law of thermodynamics. We also verify that all the configurations satisfy
an anisotropic higher-dimensional version of the Smarr formula.
