  Energy correlations characterize the energy flux through detectors at
infinity produced in a collision event. Remarkably, in holographic conformal
field theories, they probe high-energy gravitational scattering in the dual
anti-de Sitter geometry. We use known properties of high-energy gravitational
scattering and its unitarization to explore the leading quantum-gravity
correction to the energy-energy correlator at strong coupling. We find that it
includes a part originating from large impact parameter scattering that is
non-analytic in the angle between detectors and is $\log N_c$ enhanced compared
to the standard $1/N_c$ perturbative expansion. It is sensitive to the full
bulk geometry, including the internal manifold, providing a refined probe of
the emergent holographic spacetime. Similarly, scattering at small impact
parameters leads to contributions that are further enhanced by extra powers of
the 't Hooft coupling assuming it is corrected by stringy effects. We conclude
that energy correlations are sensitive to the UV properties of the dual
gravitational theory and thus provide a promising target for the conformal
bootstrap.
