  We analyze stationary BPS black hole solutions to 4d $\mathcal{N}=2$ abelian
gauged supergravity. Using an appropriate near horizon ansatz, we construct
rotating attractors with magnetic flux realizing a topological twist along the
horizon surface, for any theory with a symmetric scalar manifold. An analytic
flow to asymptotically locally $AdS_4$ is presented for a subclass of these
near horizon geometries, and an explicit new example of supersymmetric $AdS_4$
rotating black hole is discussed in detail. We further note that, upon tuning
the gauging to special values, one can obtain solutions with different
asymptotics, and in particular reductions of doubly spinning asymptotically
$AdS_5$ black holes. Finally we present a proposal for the form of the BPS
entropy function with rotation, which we expect to be holographically related
to the refined twisted index of the dual theory.
