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28 March 2024
 
  » arxiv » 1502.3287

 Article overview


Gamma-ray performance of the GAMMA-400 detector
P.Cumani ; A.M. Galper ; V. Bonvicini ; N.P. Topchiev ; O. Adriani ; R.L. Aptekar ; I.V. Arkhangelskaja ; A.I. Arkhangelskiy ; L. Bergstrom ; E. Berti ; G. Bigongiari ; S.G. Bobkov ; M. Boezio ; E.A. Bogomolov ; S. Bonechi ; M. Bongi ; S. Bottai ; G. Castellini ; P.W. Cattaneo ; G.L. Dedenko ; C. De Donato ; V.A. Dogiel ; M.S. Gorbunov ; Yu.V. Gusakov ; B.I. Hnatyk ; V.V. Kadilin ; V.A. Kaplin ; A.A. Kaplun ; M.D. Kheymits ; V.E. Korepanov ; J. Larsson ; A.A. Leonov ; V.A. Loginov ; F. Longo ; P. Maestro ; P.S. Marrocchesi ; A.L. Menshenin ; V.V. Mikhailov ; E. Mocchiutti ; A.A. Moiseev ; N. Mori ; I.V. Moskalenko ; P.Yu. Naumov ; P. Papini ; M. Pearce ; P. Picozza ; A.V. Popov ; A. Rappoldi ; S. Ricciarini ; M.F. Runtso ; F. Ryde ; R.Sarkar ; O.V. Serdin ; R. Sparvoli ; P. Spillantini ; S.I. Suchkov ; M. Tavani ; A.A. Taraskin ; A. Tiberio ; E.M. Tyurin ; M.V. Ulanov ; A. Vacchi ; E. Vannuccini ; G.I. Vasilyev ; Yu.T. Yurkin ; N. Zampa ; V.N. Zirakashvili ; V.G. Zverev ;
Date 11 Feb 2015
AbstractGAMMA-400 is a new space mission, designed as a dual experiment, capable to study both high energy gamma rays (from $sim$100 MeV to few TeV) and cosmic rays (electrons up to 20 TeV and nuclei up to $sim$10$^{15}$ eV). The full simulation framework of GAMMA-400 is based on the Geant4 toolkit. The details of the gamma-ray reconstruction pipeline in the three main instruments (Tracker, Imaging Calorimeter, Homogeneous Calorimeter) will be outlined. The performance of GAMMA-400 (PSF, effective area and sensitivity) have been obtained using this framework. The most updated results on them will be shown.
Source arXiv, 1502.3287
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