  We consider the reconstruction of a Lifshitz spacetime from three
perspectives: differential entropy (or "hole-ography"), causal wedges and
entanglement wedges. We find that not all time-varying bulk curves in vacuum
Lifshitz can be reconstructed via the differential entropy approach, adding a
caveat to the general analysis of \cite{Headrick:2014eia}. We show that the
causal wedge for Lifshitz spacetimes degenerates, while the entanglement wedge
requires the additional consideration of a set of boundary-emanating
light-sheets. The need to include bulk surfaces with no clear field theory
interpretation in the differential entropy construction and the change in the
entanglement wedge formation both serve as warnings against a naive application
of holographic entanglement entropy proposals in Lifshitz spacetimes.
