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We study the uplift of a 4d black hole in 4d Einstein–Maxwell supergravity with a spindle horizon to massive type IIA and 11d supergravity on . The solutions exhibit features distinct to the uplift of the same 4d solution to 11d supergravity on an . In particular, whereas the orbifold singularities may be removed in the 11d uplift on an , they are always present in both of the classes considered here. We compute the free energy of the solutions giving predictions for the free energy of a class of 3d Chern–Simons theories wrapped on a spindle.

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