  In this paper we numerically construct localised black hole solutions at the
IR bottom of the confining geometry of the AdS soliton. These black holes
should be thought as the finite size analogues of the domain wall solutions
that have appeared previously in the literature. From the dual CFT point of
view, these black holes correspond to finite size balls of deconfined plasma
surrounded by the confining vacuum. The plasma ball solutions are parametrised
by the temperature. For temperatures well above the deconfinement transition,
the dual black holes are small and round and they are well-described by the
asymptotically flat Schwarzschild solution. On the other hand, as the
temperature approaches the deconfinement temperature, the black holes look like
pancakes which are extended along the IR bottom of the space-time. On top of
these backgrounds, we compute various probes of confinement/deconfinement such
as temporal Wilson loops and entanglement entropy.
