  Gamma-ray lines are traditional smoking gun signatures for dark matter
annihilation in the Universe. In regions optimized for large signal-to-noise
ratio, we identified a signal candidate for a gamma-ray line at energies around
130 GeV with a post-trials significance of 3.2\sigma. Spectral and spatial
properties are not inconsistent with a dark matter signal. One year has passed
since the initial papers, and I give here a brief summary and an update on the
status of the 130 GeV feature in the un-reprocessed P7 gamma-ray data of the
Fermi-LAT.
