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Despite the diculties due to the location of the experiment at the center of the scientic payload, ef- forts have been made to determine BeppoSAX Gamma{ Ray Burst Monitor detectors response functions by means of extensive on{ground calibrations, Monte Carlo simula- tions and in{flight testing. Satisfactory results have been obtained particularly for the two detectors co{aligned with the two Wide Field Cameras (WFC, 1:5 26 keV) on{ board the same satellite, allowing nearly unprecedented broad band (1:5 700 keV) spectral analysis of events detected by both experiments.

Spectral analysis of GRB with the gamma–ray burst monitor on–board BeppoSAX