Author/Authors :
Barbiellini، نويسنده , , G. and Boezio، نويسنده , , M. and Casolino، نويسنده , , M. and Candusso، نويسنده , , M. and De Pascale، نويسنده , , M.P. and Morselli، نويسنده , , A. and Picozza، نويسنده , , P. E. Ricci، نويسنده , , M. and Sparvoli، نويسنده , , R. and Spillantini، نويسنده , , P. and Vacchi، نويسنده , , A.، نويسنده ,
Abstract :
In this article a new technique for the realization of a high energy gamma-ray telescope is presented, based on the adoption of silicon strip detectors and lead scintillating fibers. The simulated performances of such an instrument (GILDA) are significatively better than those of EGRET, the last successful experiment of a high energy gamma-ray telescope, launched on the CGRO satellite, though having less volume and weight.
