  Entanglement islands play a crucial role in our understanding of how Hawking
radiation encodes information in a black hole, but their relevance in
cosmological spacetimes is less clear. In this paper, we continue our
investigation of information recovery in de Sitter space and construct a
two-dimensional model of gravity containing a domain wall that interpolates
between de Sitter space and Rindler space. The Rindler wedges introduce
weakly-gravitating asymptotic regions from which de Sitter space can be probed,
yielding an outside perspective of the cosmological horizon. In contrast to
earlier works, backreaction effects are under control by considering a quantum
state that only breaks the thermal equilibrium of the Bunch-Davies state for a
finite time. This allows information to be decoded from the Gibbons-Hawking
radiation in a controlled fashion.
