Author/Authors :
Bartoli، نويسنده , , B. and Bastieri، نويسنده , , D. and Bigongiari، نويسنده , , C. and Ciocci، نويسنده , , M.A. and Cosulich، نويسنده , , D. and Cresti، نويسنده , , M. and Dokoutchaeva، نويسنده , , V. and Kartashov، نويسنده , , D. and Liello، نويسنده , , F. and Malakhov، نويسنده , , N. and Mariotti، نويسنده , , M. and Marsella، نويسنده , , G. and Menzione، نويسنده , , A. and Paoletti، نويسنده , , R. and Parlavecchio، نويسنده , , G، نويسنده ,
Abstract :
The CLUE experiment studies primary cosmic rays (E≥2 TeV) by detecting UV (190–230 nm) Cherenkov light produced by atmospheric showers. Since atmospheric absorption in the UV range is higher than in the visible range, CLUE cannot apply algorithms normally used in IACT11The Imaging Atmospheric Cherenkov Telescope.
iments to determine primary cosmic-ray direction. In this paper, we present a new method developed by CLUE. The algorithm performances were evaluated using simulated showers. Preliminary results of the source analysis using this new method are shown.
