First Results From the HESS Experiment with an Analysis Method Based on a Semi-analytical Shower Model

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Scientific paper

Applications of the analysis method developed for the CAT experiment (Cerenkov At Themis) which has been adapted for mono-telescope and stereoscopic observations with HESS are reported. This method is based on an analytical model giving the longitudinal and transverse light distribution resulting from the development of a gamma-ray initiated shower in the atmosphere in the focal plane of each of the cameras. It simultaneously determines the energy of the initiating gamma-ray, the position of the shower axis with respect to the detector, and the source location (gamma-ray origin) on a shower-by-shower basis. Results of this method applied to HESS experimental data and a preliminary spectrum from Crab Nebula are shown.

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