  Fifteen months of cumulative CoGeNT data are examined for indications of an
annual modulation, a predicted signature of Weakly Interacting Massive Particle
(WIMP) interactions. Presently available data support the presence of a
modulated component of unknown origin, with parameters prima facie compatible
with a galactic halo composed of light-mass WIMPs. Unoptimized estimators yield
a statistical significance for a modulation of ~2.8 sigma, limited by the short
exposure.
