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Deconvolution of Energy Spectra in the ATIC ExperimentThe Advanced Thin Ionization Calorimeter (ATIC) balloon-borne experiment is designed to perform cosmic- ray elemental spectra measurements from below 100 GeV up to tens TeV for nuclei from hydrogen to iron. The instrument is composed of a silicon matrix detector followed by a carbon target, interleaved with scintillator tracking layers, and a segmented BGO calorimeter composed of 320 individual crystals totalling 18 radiation lengths, used to determine the particle energy. The technique for deconvolution of the energy spectra measured in the thin calorimeter is based on detailed simulations of the response of the ATIC instrument to different cosmic ray nuclei over a wide energy range. The method of deconvolution is described and energy spectrum of carbon obtained by this technique is presented.
Document ID
20050215576
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Batkov, K. E.
(Moscow State Univ. Russia)
Panov, A. D.
(Moscow State Univ. Russia)
Adams, J. H.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ahn, H. S.
(Maryland Univ. College Park, MD, United States)
Bashindzhagyan, G. L.
(Moscow State Univ. Russia)
Chang, J.
(Max-Plank-Inst. for Solar System Research Lindau, Germany)
Christl, M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Fazley, A. R.
(Southern Univ. Baton Rouge, LA, United States)
Ganel, O.
(Maryland Univ. College Park, MD, United States)
Gunasigha, R. M.
(Southern Univ. Baton Rouge, LA, United States)
Guzik, T. G.
(Louisiana State Univ. Baton Rouge, LA, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2005
Subject Category
Astrophysics
Meeting Information
Meeting: 29th International Cosmic Ray Conference
Location: Pune
Country: India
Start Date: August 3, 2005
End Date: August 10, 2005
Distribution Limits
Public
Copyright
Other

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