  We construct an effective field theory (EFT) description of the hard photon
spectrum for heavy WIMP annihilation. This facilitates precision predictions
relevant for line searches, and allows the incorporation of non-trivial energy
resolution effects. Our framework combines techniques from non-relativistic
EFTs and soft-collinear effective theory (SCET), as well as its multi-scale
extensions that have been recently introduced for studying jet substructure. We
find a number of interesting features, including the simultaneous presence of
SCET$_{\text{I}}$ and SCET$_{\text{II}}$ modes, as well as collinear-soft modes
at the electroweak scale. We derive a factorization formula that enables both
the resummation of the leading large Sudakov double logarithms that appear in
the perturbative spectrum, and the inclusion of Sommerfeld enhancement effects.
Consistency of this factorization is demonstrated to leading logarithmic order
through explicit calculation. Our final result contains both the exclusive and
the inclusive limits, thereby providing a unifying description of these two
previously-considered approximations. We estimate the impact on experimental
sensitivity, focusing for concreteness on an SU(2)$_{W}$ triplet fermion dark
matter - the pure wino - where the strongest constraints are due to a search
for gamma-ray lines from the Galactic Center. We find numerically significant
corrections compared to previous results, thereby highlighting the importance
of accounting for the photon spectrum when interpreting data from current and
future indirect detection experiments.
