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A new approach to Gamma/Hadron separation algorithms is proposed. Thedifferences between Gamma and Hadron showers are notorious in two main aspects.The first is the wideness of the shower, and the second is the distribution ofthe angles of emission of Cherenkov photons in respect to the shower main axis.Using more than one IAC telescope, and their respective bi-dimensional imagesof arrival directions of the Cherenkov photons, the 3D geometricalcharacteristics of the shower can be reconstructed.

Gamma/hadron separation in IACTs using 3D EAS variables