  We construct charged and rotating asymptotically Schrodinger black hole
solutions of IIB supergravity. We begin by obtaining a closed-form expression
for the null Melvin twist of a broad class of type IIB backgrounds, including
solutions of minimal five-dimensional gauged supergravity, and identify the
resulting five-dimensional effective action. We use these results to
demonstrate that the near-horizon physics and thermodynamics of asymptotically
Schrodinger black holes obtained in this way are essentially inherited from
their AdS progenitors, and verify that they admit zero-temperature extremal
limits with AdS_2 near-horizon geometries. Notably, the AdS_2 radius is
parametrically larger than that of the asymptotic Schrodinger space.
