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Developments and results in the context of the JEM-EUSO program obtained with the ESAF simulation and analysis framework

  • S. Abe
  • , J. H. Adams
  • , D. Allard
  • , P. Alldredge
  • , L. Anchordoqui
  • , A. Anzalone
  • , E. Arnone
  • , B. Baret
  • , D. Barghini
  • , M. Battisti
  • , J. Bayer
  • , R. Bellotti
  • , A. A. Belov
  • , M. Bertaina
  • , P. F. Bertone
  • , M. Bianciotto
  • , P. L. Biermann
  • , F. Bisconti
  • , C. Blaksley
  • , S. Blin-Bondil
  • P. Bobik, K. Bolmgren, S. Briz, J. Burton, F. Cafagna, G. Cambié, D. Campana, F. Capel, R. Caruso, M. Casolino, C. Cassardo, A. Castellina, K. Černý, M. J. Christl, R. Colalillo, L. Conti, G. Cotto, H. J. Crawford, R. Cremonini, A. Creusot, A. Cummings, A. de Castro Gónzalez, C. de la Taille, L. del Peral, R. Diesing, P. Dinaucourt, A. Di Nola, A. Ebersoldt, T. Ebisuzaki, J. Eser, F. Fenu, S. Ferrarese, G. Filippatos, W. W. Finch, F. Flaminio, C. Fornaro, D. Fuehne, C. Fuglesang, M. Fukushima, D. Gardiol, G. K. Garipov, A. Golzio, P. Gorodetzky, F. Guarino, C. Guépin, A. Guzmán, A. Haungs, T. Heibges, J. Hernández-Carretero, F. Isgrò, E. G. Judd, F. Kajino, I. Kaneko, Y. Kawasaki, M. Kleifges, P. A. Klimov, I. Kreykenbohm, J. F. Krizmanic, V. Kungel, E. Kuznetsov, F. López Martínez, S. Mackovjak, D. Mandát, M. Manfrin, A. Marcelli, L. Marcelli, W. Marszał, J. N. Matthews, A. Menshikov, T. Mernik, M. Mese, S. S. Meyer, J. Mimouni, H. Miyamoto, Y. Mizumoto, A. Monaco, J. A. Morales de los Ríos, S. Nagataki, J. M. Nachtman, D. Naumov, A. Neronov, T. Nonaka, T. Ogawa, S. Ogio, H. Ohmori, A. V. Olinto, Y. Onel, G. Osteria, A. Pagliaro, B. Panico, E. Parizot, I. H. Park, B. Pastircak, T. Paul, M. Pech, F. Perfetto, P. Picozza, L. W. Piotrowski, Z. Plebaniak, J. Posligua, R. Prevete, G. Prévôt, H. Prieto, M. Przybylak, M. Putis, E. Reali, P. Reardon, M. H. Reno, M. Ricci, M. Rodríguez Frías, G. Romoli, G. Sáez Cano, H. Sagawa, N. Sakaki, A. Santangelo, O. A. Saprykin, F. Sarazin, M. Sato, H. Schieler, P. Schovánek, V. Scotti, S. Selmane, S. A. Sharakin, K. Shinozaki, J. F. Soriano, J. Szabelski, N. Tajima, T. Tajima, Y. Takahashi, M. Takeda, Y. Takizawa, C. Tenzer, S. B. Thomas, L. G. Tkachev, T. Tomida, S. Toscano, M. Traïche, D. Trofimov, K. Tsuno, P. Vallania, L. Valore, T. M. Venters, C. Vigorito, P. von Ballmoos, M. Vrabel, S. Wada, J. Watts, A. Weindl, L. Wiencke, J. Wilms, D. Winn, H. Wistrand, I. V. Yashin, R. Young, M. Yu Zotov
  • Nihon University
  • University of Alabama in Huntsville
  • Astroparticule and Cosmol APC
  • Lehman College
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
  • INFN Sezione di Catania
  • INFN Sezione di Torino
  • University of Turin
  • University of Tübingen
  • INFN Sezione di Bari
  • Università degli studi di Bari Aldo Moro
  • Moscow State University
  • NASA Marshall Space Flight Center
  • Institute of Meteorology and Climate Research
  • INFN Roma Tor Vergata
  • Riken
  • Institute of Experimental Physics Slovak Academy of Sciences
  • KTH Royal Institute of Technology
  • University of Chicago
  • University of Rome “Tor Vergata”
  • INFN Sezione di Napoli
  • Max-Planck-Institut für Physik
  • Università degli Studi di Catania
  • Istituto di Astrofisica e Planetologia Spaziali (IAPS)
  • Joint Laboratory of Optics
  • University of Naples Federico II
  • UTIU
  • University of California, Space Sciences Laboratory
  • Pennsylvania State University
  • Universidad de Alcalá
  • Science and Research Directorate
  • Colorado School of Mines
  • University of Tokyo
  • Konan University
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • NASA Goddard Space Flight Center
  • Institute of Physics of the Czech Academy of Sciences
  • National Centre for Nuclear Research
  • University of Utah
  • Univ. Mentouri de Constantine
  • National Astronomical Observatory
  • University of Iowa
  • Joint Institute for Nuclear Research, Dubna
  • Institut Universitaire de France
  • Sungkyunkwan University
  • University of Warsaw
  • LNF-INFN
  • Parque Científico USAL
  • Space Regatta Consortium
  • Hokkaido University
  • Long Beach VA and University of California
  • Shinshu University
  • University of Geneva
  • Centre de Développement des Technologies Avancées
  • IRAP/CNRS
  • Fairfield University

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12 Citations (Scopus)

Résumé

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 ESAF in 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.

langue originaleAnglais
Numéro d'article1028
journalEuropean Physical Journal C
Volume83
Numéro de publication11
Les DOIs
étatPublié - 1 nov. 2023

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