Performances of JEM-EUSO: energy and X

The Extreme Universe Space Observatory (EUSO) on-board the Japanese Experimental Module (JEM) of the International Space Station aims at the detection of ultra high energy cosmic rays from space. The mission consists of a UV telescope which will detect the fluorescence light emitted by cosmic ray sh...

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Veröffentlicht in:Experimental astronomy 2015-11, Vol.40 (1), p.183-214
Hauptverfasser: Adams, JH Jr, Ahmad, S, Albert, J-N, Allard, D, Anchordoqui, L, Andreev, V, Anzalone, A, Arai, Y, Asano, K, Pernas, MAve, Baragatti, P, Barrillon, P, Batsch, T, Bayer, J, Bechini, R, Belenguer, T, Bellotti, R, Belov, K, Berlind, A A, Bertaina, M, Biermann, P L, Biktemerova, S, Blaksley, C, Blanc, N, Blecki, J, Blin-Bondil, S, Bluemer, J, Bobik, P, Bogomilov, M, Bonamente, M, Briggs, MS, Briz, S, Bruno, A, Cafagna, F, Campana, D, Capdevielle, J-N, Caruso, R, Casolino, M, Cassardo, C, Castellinic, G, Catalano, C, Catalano, G, Cellino, A, Chikawa, M, Christl, MJ, Cline, D, Connaughton, V, Conti, L, Cordero, G, Crawford, HJ, et. al
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container_end_page 214
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container_title Experimental astronomy
container_volume 40
creator Adams, JH Jr
Ahmad, S
Albert, J-N
Allard, D
Anchordoqui, L
Andreev, V
Anzalone, A
Arai, Y
Asano, K
Pernas, MAve
Baragatti, P
Barrillon, P
Batsch, T
Bayer, J
Bechini, R
Belenguer, T
Bellotti, R
Belov, K
Berlind, A A
Bertaina, M
Biermann, P L
Biktemerova, S
Blaksley, C
Blanc, N
Blecki, J
Blin-Bondil, S
Bluemer, J
Bobik, P
Bogomilov, M
Bonamente, M
Briggs, MS
Briz, S
Bruno, A
Cafagna, F
Campana, D
Capdevielle, J-N
Caruso, R
Casolino, M
Cassardo, C
Castellinic, G
Catalano, C
Catalano, G
Cellino, A
Chikawa, M
Christl, MJ
Cline, D
Connaughton, V
Conti, L
Cordero, G
Crawford, HJ
et. al
description The Extreme Universe Space Observatory (EUSO) on-board the Japanese Experimental Module (JEM) of the International Space Station aims at the detection of ultra high energy cosmic rays from space. The mission consists of a UV telescope which will detect the fluorescence light emitted by cosmic ray showers in the atmosphere. The mission, currently developed by a large international collaboration, is designed to be launched within this decade. In this article, we present the reconstruction of the energy of the observed events and we also address the X sub(max) reconstruction. After discussing the algorithms developed for the energy and X sub(max) reconstruction, we present several estimates of the energy resolution, as a function of the incident angle, and energy of the event. Similarly, estimates of the X sub(max) resolution for various conditions are presented.
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subjects Algorithms
Astronomy
Cooperation
Cosmic rays
Estimates
Missions
Reconstruction
Universe
title Performances of JEM-EUSO: energy and X
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