Developments and results in the context of the JEM-EUSO program obtained with the ESAF Simulation and Analysis Framework
Instrumentation and Methods for Astrophysics
2023-11-22 v1 High Energy Physics - Experiment
Abstract
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.
Keywords
Cite
@article{arxiv.2311.12656,
title = {Developments and results in the context of the JEM-EUSO program obtained with the ESAF Simulation and Analysis Framework},
author = {S. Abe and J. H. Adams and D. Allard and P. Alldredge and L. Anchordoqui and A. Anzalone and E. Arnone and B. Baret and D. Barghini and M. Battisti and J. Bayer and R. Bellotti and A. A. Belov and M. Bertaina and P. F. Bertone and M. Bianciotto and P. L. Biermann and F. Bisconti and C. Blaksley and S. Blin-Bondil and P. Bobik and K. Bolmgren and S. Briz and J. Burton and F. Cafagna and G. Cambié and D. Campana and F. Capel and R. Caruso and M. Casolino and C. Cassardo and A. Castellina and K. Černý and M. J. Christl and R. Colalillo and L. Conti and G. Cotto and H. J. Crawford and R. Cremonini and A. Creusot and A. Cummings and A. de Castro Gónzalez and C. de la Taille and L. del Peral and R. Diesing and P. Dinaucourt and A. Di Nola and A. Ebersoldt and T. Ebisuzaki and J. Eser and F. Fenu and S. Ferrarese and G. Filippatos and W. W. Finch and F. Flaminio and C. Fornaro and D. Fuehne and C. Fuglesang and M. Fukushima and D. Gardiol and G. K. Garipov and A. Golzio and P. Gorodetzky and F. Guarino and C. Guépin and A. Guzmán and A. Haungs and T. Heibges and J. Hernández-Carretero and F. Isgrò and E. G. Judd and F. Kajino and I. Kaneko and Y. Kawasaki and M. Kleifges and P. A. Klimov and I. Kreykenbohm and J. F. Krizmanic and V. Kungel and E. Kuznetsov and F. López Martínez and S. Mackovjak and D. Mandát and M. Manfrin and A. Marcelli and L. Marcelli and W. Marszał and J. N. Matthews and A. Menshikov and T. Mernik and M. Mese and S. S. Meyer and J. Mimouni and H. Miyamoto and Y. Mizumoto and A. Monaco and J. A Morales de los Ríos and S. Nagataki and J. M. Nachtman and D. Naumov and A. Neronov and T. Nonaka and T. Ogawa and S. Ogio and H. Ohmori and A. V. Olinto and Y. Onel and G. Osteria and A. Pagliaro and B. Panico and E. Parizot and I. H. Park and B. Pastircak and T. Paul and M. Pech and F. Perfetto and P. Picozza and L. W. Piotrowski and Z. Plebaniak and J. Posligua and R. Prevete and G. Prévôt and H. Prieto and M. Przybylak and M. Putis and E. Reali and P. Reardon and M. H. Reno and M. Ricci and M. Rodríguez Frías and G. Romoli and G. Sáez Cano and H. Sagawa and N. Sakaki and A. Santangelo and O. A. Saprykin and F. Sarazin and M. Sato and H. Schieler and P. Schovánek and V. Scotti and S. Selmane and S. A. Sharakin and K. Shinozaki and J. F. Soriano and J. Szabelski and N. Tajima and T. Tajima and Y. Takahashi and M. Takeda and Y. Takizawa and C. Tenzer and S. B. Thomas and L. G. Tkachev and T. Tomida and S. Toscano and M. Traïche and D. Trofimov and K. Tsuno and P. Vallania and L. Valore and T. M. Venters and C. Vigorito and P. von Ballmoos and M. Vrabel and S. Wada and J. Watts and A. Weindl and L. Wiencke and J. Wilms and D. Winn and H. Wistrand and I. V. Yashin and R. Young and M. Yu. Zotov},
journal= {arXiv preprint arXiv:2311.12656},
year = {2023}
}