The GILDA mission: a new technique for a gamma-ray telescope in the energy range 20 MeV-100 GeV

Details The GILDA mission: a new technique for a gamma-ray telescope in the energy range 20 MeV-100 GeV The GILDA mission: a new technique for a gamma-ray telescope in the energy range 20 MeV-100 GeV

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995nimpa.354..547b&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, v. 354, p. 547-552

Physics

15

Scientific paper

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.

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