  The maximal four-dimensional supergravity with a dyonic ISO(7) gauging that
arises from the reduction of massive IIA on a six-sphere has recently been
shown to accommodate static BPS black holes with hyperbolic horizons. When
restricted to the N=2 subsector that retains one vector multiplet and the
universal hypermultiplet, the attractor mechanism was shown to fix both the
vector charges and the scalar fields at the horizon to a unique configuration
in terms of the gauging parameters. In order to assess the (non-)uniqueness of
BPS black hole horizons from massive IIA, we extend the study of the attractor
mechanism to other N=2 subsectors including additional matter multiplets. We
note that, while extending the hypermultiplet sector does not modify the set of
solutions to the attractor equations, the inclusion of additional vector
multiplets results in new hyperbolic/spherical horizons containing free
parameters. The model with three vector multiplets and the universal
hypermultiplet, which is the massive IIA analogue of the STU-model from
M-theory, may play a relevant role in massive IIA holography.
