Heaton C, Abdellaoui G, Abe S, Adams JH, Allard D, Alonso G, Anchordoqui L, Anzalone A, Arnone E, Asano K, Attallah R, Attoui H, Ave Pernas M, Bagheri M, Baláz J, Bakiri M, Barghini D, Bartocci S, Battisti M, Bayer J, Beldjilali B, Belenguer T, Belkhalfa N, Bellotti R, Belov AA, Benmessai K, Bertaina M, Bertone PF, Biermann PL, Bisconti F, Blaksley C, Blanc N, Blin-Bondil S, Bobik P, Bogomilov M, Bolmgren K, Bozzo E, Briz S, Bruno A, Caballero KS, Cafagna F, Cambié G, Campana D, Capdevielle JN, Capel F, Caramete A, Caramete L, Carlson P, Caruso R, Casolino M, Cassardo C, Castellina A, Catalano O, Cellino A, Černý K, Chikawa M, Chiritoi G, Christl MJ, Colalillo R, Conti L, Cotto G, Crawford HJ, Cremonini R, Creusot A, de Castro Gónzalez A, de la Taille C, del Peral L, Diaz Damian A, Diesing R, Dinaucourt P, Djakonow A, Djemil T, Ebersoldt A, Ebisuzaki T, Eser J, Fenu F, Fernández-González S, Ferrarese S, Filippatos G, Finch WI, Fornaro C, Fouka M, Franceschi A, Franchini S, Fuglesang C, Fujii T, Fukushima M, Galeotti P, García-Ortega E, Gardiol D, Garipov GK, Gascón E, Gazda E, Genci J, Golzio A, González Alvarado C, Gorodetzky P, Green A, Guarino F, Guépin C, Guzmán A, Hachisu Y, Haungs A, Hernández Carretero J, Hulett L, Ikeda D, Inoue N, Inoue S, Isgrò F, Itow Y, Jammer T, Jeong S, Joven E, Judd EG, Jochum J, Kajino F, Kajino T, Kalli S, Kaneko I, Karadzhov Y, Kasztelan M, Katahira K, Kawai K, Kawasaki Y, Kedadra A, Khales H, Khrenov BA, Kim JS, Kim SW, Kleifges M, Klimov PA, Kolev D, Kreykenbohm I, Krizmanic JF, Królik K, Kungel V, Kurihara Y, Kusenko A, Kuznetsov E, Lahmar H, Lakhdari F, Licandro J, López Campano L, López Martínez F, Mackovjak S, Mahdi M, Mandát D, Manfrin M, Marcelli L, Marcos JL, Marszał W, Martín Y, Martinez O, Mase K, Matev R, Matthews JN, Mebarki N, Medina-Tanco G, Menshikov A, Merino A, Mese M, Meseguer J, Meyer SS, Mimouni J, Miyamoto H, Mizumoto Y, Monaco A, Morales de los Ríos JA, Mastafa M, Nagataki S, Naitamor S, Napolitano T, Nachtman JM, Neronov A, Nomoto K, Nonaka T, Ogawa T, Ogio S, Ohmori H, Olinto AV, Onel Y, Osteria G, Otte AN, Pagliaro A, Painter W, Panasyuk MI, Panico B, Parizot E, Park IH, Pastircak B, Paul T, Pech M, Pérez-Grande I, Perfetto F, Peter T, Picozza P, Pindado S, Piotrowski LW, Piraino S, Plebaniak Z, Pollini A, Popescu EM, Prevete R, Prévôt G, Prieto H, Przybylak M, Puehlhofer G, Putis M, Reardon P, Reno MH, Reyes M, Ricci M, Rodríguez Frías MD, Romero Matamala OF, Ronga F, Sabau MD, Saccá G, Sáez Cano G, Sagawa H, Sahnoune Z, Saito A, Sakaki N, Salazar H, Sanchez Balanzar JC, Sánchez JL, Santangelo A, Sanz-Andrés A, Sanz Palomino M, Saprykin OA, Sarazin F, Sato M, Scagliola A, Schanz T, Schieler H, Schovánek P, Scotti V, Serra M, Sharakin SA, Shimizu HM, Shinozaki K, Soriano JF, Sotgiu A, Stan I, Strharský I, Sugiyama N, Supanitsky D, Suzuki M, Szabelski J, Tajima N, Tajima T, Takahashi Y, Takeda M, Takizawa Y, Talai MC, Tameda Y, Tenzer C, Thomas SB, Tibolla O, Tkachev LG, Tomida T, Tone N, Toscano S, Traïche M, Tsunesada Y, Tsuno K, Turriziani S, Uchihori Y, Vaduvescu O, Valdés-Galicia JF, Vallania P, Valore L, Vankova-Kirilova G, Venters TM, Vigorito C, Villaseñor L, Vlcek B, von Ballmoos P, Vrabel M, Wada S, Watanabe J, Watts J, Weigand Muñoz R, Weindl A, Wiencke L, Wille M, Wilms J, Winn D, Yamamoto T, Yang J, Yano H, Yashin IV, Yonetoku D, Yoshida S, Young R, Zgura IS, Zotov MY, Zuccaro Marchi A (2022)
Publication Type: Conference contribution
Publication year: 2022
Publisher: Sissa Medialab Srl
Book Volume: 395
Conference Proceedings Title: Proceedings of Science
Event location: Virtual, Berlin, DEU
The Extreme Universe Space Observatory Super Pressure Balloon 2 (EUSO-SPB2) is under development, and will prototype instrumentation for future satellite-based missions, including the Probe of Extreme Multi-Messenger Astrophysics (POEMMA). EUSO-SPB2 will consist of two telescopes. The first is a Cherenkov telescope (CT) being developed to identify and estimate the background sources for future below-the-limb very high energy (E>10 PeV) astrophysical neutrino observations, as well as above-the-limb cosmic ray induced signals (E>1 PeV). The second is a fluorescence telescope (FT) being developed for detection of Ultra High Energy Cosmic Rays (UHECRs). In preparation for the expected launch in 2023, extensive simulations tuned by preliminary laboratory measurements have been performed to understand the FT capabilities. The energy threshold has been estimated at 1018.2 eV, and results in a maximum detection rate at 1018.6 eV when taking into account the shape of the UHECR spectrum. In addition, onboard software has been developed based on the simulations as well as experience with previous EUSO missions. This includes a level 1 trigger to be run on the computationally limited flight hardware, as well as a deep learning based prioritization algorithm in order to accommodate the balloon's telemetry budget. These techniques could also be used later for future, space-based missions.
APA:
Heaton, C., Abdellaoui, G., Abe, S., Adams, J.H., Allard, D., Alonso, G.,... Zuccaro Marchi, A. (2022). Expected Performance of the EUSO-SPB2 Fluorescence Telescope. In Proceedings of Science. Virtual, Berlin, DEU: Sissa Medialab Srl.
MLA:
Heaton, C., et al. "Expected Performance of the EUSO-SPB2 Fluorescence Telescope." Proceedings of the 37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin, DEU Sissa Medialab Srl, 2022.
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