By M. Barone
Lawsuits of the seventh foreign convention on ICATPP-7, held October 15-19, 2001 in Villa, Olmo, Como, Italy. gains brand new expertise purposes to radiation detection.
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3rd E G R E T catalog for sources of energies greater than 100 MeV. of the sources result still unidentified. The majority and for annihilations of postulated weakly-interacting massive particles (or WIMPs). Most of the isotropic background measured by EGRET will be resolved by GLAST as diffuse emissions from AGN. A diffuse cosmic residual would be a tremendous discovery and could be related to strange particle decay. Recent work suggests that annihilation of the lightest supersymmetric particles, a candidate Galactic Halo WIMP, could leave a signature in the diffuse background detectable by GLAST.
Sagnac, Compt. Rend. Acad. Sci. 157, 708 (1913). THE GLAST G A M M A RAY LARGE A R E A TELESCOPE S. BREZ, R. N. OMODEI, N. LUMB, L. BALDINI, L. LATRONICO INFN Sez. Pisa Via Livornese 1291 56010 S. Piero a Grado (Pisa) For the Italian GLAST Collaboration The Gamma-ray Large Area Space Telescope (GLAST) is an international space mission that will study the cosmos in the energy range 10 KeV — 300 GeV, the upper end of which is one of the last poorly observed regions of the celestial electromagnetic spectrum to be explored.
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