  Modern meta-materials allow one to construct electromagnetic media with
almost arbitrary bespoke permittivity, permeability, and magneto-electric
tensors. If (and only if) the permittivity, permeability, and magneto-electric
tensors satisfy certain stringent compatibility conditions, can the
meta-material be fully described (at the wave optics level) in terms of an
effective Lorentzian metric --- an analogue spacetime. We shall consider some
of the standard black-hole spacetimes of primary interest in general
relativity, in various coordinate systems, and determine the equivalent
meta-material susceptibility tensors in a laboratory setting. In static black
hole spacetimes (Schwarzschild and the like) certain eigenvalues of the
susceptibility tensors will be seen to diverge on the horizon. In stationary
black hole spacetimes (Kerr and the like) certain eigenvalues of the
susceptibility tensors will be seen to diverge on the ergo-surface.
