Study of the Gamma-ray performance of the GAMMA-400 Calorimeter

P.Cumani , A.M. Galper , V. Bonvicini , N.P. Topchiev , O. Adriani , R.L. Aptekar , A. Argan , I.V. Arkhangelskaja

show 68 more authors

A.I. Arkhangelskiy L. Bergstrom E. Berti G. Bigongiari S.G. Bobkov M. Boezio E.A. Bogomolov S. Bonechi M. Bongi S. Bottai A. Bulgarelli G. Castellini P.W. Cattaneo G.L. Dedenko C. De Donato V.A. Dogiel I. Donnarumma V. Fioretti 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 F. Palma P. Papini M. Pearce G. Piano P. Picozza A.V. Popov A. Rappoldi S. Ricciarini M.F. Runtso F. Ryde S. Sabatini 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 V. Vittorini Yu.T. Yurkin N. Zampa V.N. Zirakashvili V.G. Zverev

Authors on Pith no claims yet

classification 🌌 astro-ph.IM astro-ph.HE

keywords gamma-400calorimeterframeworkgamma-rayperformancerayswillarea

0 comments

read the original abstract

GAMMA-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 pre-shower and calorimeter will be outlined. The performance of GAMMA-400 (PSF, effective area) have been obtained using this framework. The most updated results on them will be shown.

This paper has not been read by Pith yet.

Study of the Gamma-ray performance of the GAMMA-400 Calorimeter

discussion (0)