  We construct a supersymmetric rotating black hole with asymptotically flat
four-dimensional spacetime times a circle, by superposing an infinite number of
BMPV black hole solutions at the same distance in one direction. The near
horizon structure is the same as that of the five-dimensional BMPV black hole.
The rotation of this black hole can exceed the Kerr bound in general relativity
($q\equiv a/G_4 M=1$), if the size is small.
