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

Search for an Annual Modulation in a P-type Point Contact Germanium Dark Matter Detector