  In arbitrary dimension, we consider the Einstein-Maxwell Lagrangian
supplemented by the more general quadratic-curvature corrections. For this
model, we derive four classes of charged Lifshitz black hole solutions for
which the metric function is shown to depend on a unique integration constant.
The masses of these solutions are computed using the quasilocal formalism based
on the relation established between the off-shell ADT and Noether potentials.
Among these four solutions, three of them are interpreted as extremal in the
sense that their mass vanishes identically. For the last family of solutions,
the quasilocal mass and the electric charge both are shown to depend on the
integration constant. Finally, we verify that the first law of thermodynamics
holds for each solution and a Smarr formula is also established for the four
solutions.
