  We study the reflected entropy $S_R$ in the West Coast Model, a toy model of
black hole evaporation consisting of JT gravity coupled to end-of-the-world
branes. We demonstrate the validity of the holographic duality relating it to
the entanglement wedge cross section away from phase transitions. Further, we
analyze the important non-perturbative effects that smooth out the
discontinuity in the $S_R$ phase transition. By performing the gravitational
path integral, we obtain the reflected entanglement spectrum analytically. The
spectrum takes a simple form consisting of superselection sectors, which we
interpret as a direct sum of geometries, a disconnected one and a connected one
involving a closed universe. We find that area fluctuations of $O(\sqrt{G_N})$
spread out the $S_R$ phase transition in the canonical ensemble, analogous to
the entanglement entropy phase transition. We also consider a Renyi
generalization of the reflected entropy and show that the location of the phase
transition varies as a function of the Renyi parameter.
