  In this paper we study the thermodynamics of rotating black hole solutions
arising from four-dimensional gauged N=2 supergravity. We analyze two different
supergravity models, characterized by prepotentials $F = -i X^0 X^1$ and $F=
-2i \sqrt{X^0 (X^1)^3}$. The black hole configurations are supported by
electromagnetic charges and scalar fields with different kinds of boundary
conditions. We perform our analysis in the canonical ensemble, where we find a
first order phase transition for a suitable range of charges and angular
momentum. We perform the thermodynamic stability check on the configurations.
Using the holographic dictionary we interpret the phase transition in terms of
expectation values of operators in the dual field theory, which pertains to the
class of ABJM theories living on a rotating Einstein universe. We extend the
analysis to dyonic configurations as well. Lastly, we show the computation of
the on-shell action and mass via holographic renormalization techniques.
