Abstract
Gamma-telescope GAMMA-400 consists of anticoincidence system (polyvinylyltoluene BC-408 based top and lateral detector sections, the converter-tracker with thickness of ∼1 X0 (where X0 is radiation length), time-of-flight system (two sections composed of BC-408 detectors with 50cm distance between), two calorimeters makes of CsI(Tl) crystals (position-sensitive and electromagnetic. Also it includes neutron detector, two BC-408 based scintillation detectors of the calorimeter, and four BC-408 based lateral detectors of the calorimeter. The total calorimeter thickness is 25 X0 or 1.2 λ0 for vertical incident particles registration and 54 X0 or 2.5 λ0 for laterally incident ones (where λ0 is nuclear interaction length). The counting and triggers signals formation system started the data acquisition and provides particle identification. It used 2 pulses types: fast (t≤10ns) from BC-408 based scintillation detectors and slow (t≤10ms) from inorganic ones. Also fast pulses (t∼10ns) from inorganic calorimeters individual detectors amplitude discriminators are included to this system information processing. Only signals from each detectors system individual detecting units without any summation are used for particle identification. The relationship between γ-quanta and relativistic particles (electrons and protons) energy deposition in GAMMA-400 detectors are discussed. The onboard triggers and trigger markers formation algorithms are described jointly with particles identification methods.
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