  We construct an asymptotically flat, stationary and biaxisymmetric
supersymmetric black lens solution in five-dimensional U(1)^3 supergravity. It
is shown that the spatial cross section of the horizon is topologically the
lens space of L(n,1), and the spacetime is regular on/outside the event
horizon. The black lens carries (3n+2) physical quantities, three electric
charges, two angular momenta and 3(n-1) magnetic fluxes.
