A high performance likelihood reconstruction of gamma-rays for Imaging Atmospheric Cherenkov Telescopes
Résumé
We present a sophisticated gamma-ray likelihood reconstruction technique for Imaging Atmospheric Cerenkov Telescopes. The technique is based on the comparison of the raw Cherenkov camera pixel images of a photon induced atmospheric particle shower with the predictions from a semi-analytical model. The approach was initiated by the CAT experiment in the 1990's, and has been further developed by a new fit algorithm based on a log-likelihood minimisation using all pixels in the camera, a precise treatment of night sky background noise, the use of stereoscopy and the introduction of first interaction depth as parameter of the model.
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PEER_stage2_10.1016%2Fj.astropartphys.2009.09.001.pdf (3.08 Mo)
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