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  • Developments and results in the context of the JEM-EUSO program obtained with the ESAF Simulation and Analysis Framework
    Adams, J H; Anchordoqui, L; Arnone, E; Baret, B; Barghini, D; Bellotti, R; Bertaina, M; Bertone, P F; Biermann, P L; Bisconti, F; Blaksley, C; Bobik, P; Briz, S; Burton, J; Cafagna, F; Capel, F; Caruso, R; Casolino, M; Černý, K; Colalillo, R; Conti, L; Cotto, G; Crawford, H J; Cremonini, R; Cummings, A; de la Taille, C; L del Peral; Diesing, R; Dinaucourt, P; Ebisuzaki, T; Ferrarese, S; Filippatos, G; Finch, W W; naro, C; Fuehne, D; Fuglesang, C; Garipov, G K; Gorodetzky, P; Guzmán, A; Haungs, A; Heibges, T; Isgrò, F; Judd, E G; Kaneko, I; Kawasaki, Y; Kleifges, M; Klimov, P A; Kreykenbohm, I; Krizmanic, J F; Kungel, V; Manfrin, M; Marcelli, L; Marszał, W; Meyer, S S; Miyamoto, H; Mizumoto, Y; Monaco, A; Nagataki, S; Nachtman, J M; Nonaka, T; Ogawa, T; Ohmori, H; Osteria, G; Pagliaro, A; Parizot, E; Pastircak, B; Paul, T; Picozza, P; Piotrowski, L W; Posligua, J; Prieto, H; Przybylak, M; Reali, E; Reno, M H; Ricci, M; Sagawa, H; Sakaki, N; Santangelo, A; Saprykin, O A; Schieler, H; Scotti, V; Sharakin, S A; Shinozaki, K; Soriano, J F; Szabelski, J; Tajima, N; Takahashi, Y; Takeda, M; Tenzer, C; Thomas, S B; Trofimov, D; Valore, L; Venters, T M; Vrabel, M; Wada, S; Watts, J; Weindl, A; Wiencke, L; Wistrand, H; Yashin, I V

    arXiv.org, 11/2023
    Paper, Journal Article

    JEM--EUSO is an international program for the development of space-based Ultra-High Energy Cosmic Ray observatories. The program consists of a series of missions which are either under development or in the data analysis phase. All instruments are based on a wide-field-of-view telescope, which operates in the near-UV range, designed to detect the fluorescence light emitted by extensive air showers in the atmosphere. We describe the simulation software ESAFin the framework of the JEM--EUSO program and explain the physical assumptions used. We present here the implementation of the JEM--EUSO, POEMMA, K--EUSO, TUS, Mini--EUSO, EUSO--SPB1 and EUSO--TA configurations in ESAF. For the first time ESAF simulation outputs are compared with experimental data.

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