  Recently, new holographic models of black hole evaporation have given fresh
insights into the information paradox [arXiv:1905.08255, arXiv:1905.08762,
arXiv:1908.10996]. In these models, the black hole evaporates into an auxiliary
bath space after a quantum quench, wherein the holographic theory and the bath
are joined. One particularly exciting development is the appearance of
"ER=EPR"-like wormholes in the (doubly) holographic model of
[arXiv:1908.10996]. At late times, the entanglement wedge of the bath includes
the interior of the black hole. In this paper, we employ both numerical and
analytic methods to study how information about the black hole interior is
encoded in the Hawking radiation. In particular, we systematically excise
intervals from the bath from the system and study the corresponding Page
transition. Repeating this process ad infinitum, we end up with a fractal
structure on which the black hole interior is encoded, implementing the
uberholography protocol of [arXiv:1612.00017].
