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EUSO-SPB1 mission and scienceopen access

Authors
Abdellaoui, G.Abe, S.Adams, J.H.Allard, D.Alonso, G.Anchordoqui, L.Anzalone, A.Arnone, E.Asano, K.Attallah, R.Attoui, H.Pernas, M. AveBachmann, R.Bacholle, S.Bagheri, M.Bakiri, M.Baláz, J.Barghini, D.Bartocci, S.Battisti, M.Bayer, J.Beldjilali, B.Belenguer, T.Belkhalfa, N.Bellotti, R.Belov, A.A.Benmessai, K.Bertaina, M.Bertone, P.F.Biermann, P.L.Bisconti, F.Blaksley, C.Blanc, N.Blin-Bondil, S.Bobik, P.Bogomilov, M.Bolmgren, K.Bozzo, E.Briz, S.Bruno, A.Caballero, K.S.Cafagna, F.Cambié, G.Campana, D.Capdevielle, J.N.Capel, F.Caramete, A.Caramete, L.Caruso, R.Casolino, M.Cassardo, C.Castellina, A.Catalano, O.Cellino, A.Černý, K.Chikawa, M.Chiritoi, G.Christl, M.J.Colalillo, R.Conti, L.Cotto, G.Crawford, H.J.Cremonini, R.Creusot, A.Cummings, A.de Castro Gónzalez, A.de la Taille, C.del Peral, L.Desiato, J.Damian, A. DiazDiesing, R.Dinaucourt, P.Djakonow, A.Djemil, T.Ebersoldt, A.Ebisuzaki, T.Eser, J.Fenu, F.Fernández-González, S.Ferrarese, S.Filippatos, G.Finch, W.Fornaro, C.Fouka, M.Franceschi, A.Franchini, S.Fuglesang, C.Fujii, T.Fukushima, M.Galeotti, P.García-Ortega, E.Gardiol, D.Garipov, G.K.Gascón, E.Gazda, E.Genci, J.Golzio, A.Gorodetzky, P.Gregg, R.Green, A.Guarino, F.Guépin, C.Guzmán, A.Hachisu, Y.Haungs, A.Heigbes, T.Carretero, J. HernándezHulett, L.Ikeda, D.Inoue, N.Inoue, S.Isgrò, F.Itow, Y.Jammer, T.Jeong, S.Jochum, J.Joven, E.Judd, E.G.Jung, A.Kajino, F.Kajino, T.Kalli, S.Kaneko, I.Kasztelan, M.Katahira, K.Kawai, K.Kawasaki, Y.Kedadra, A.Khales, H.Khrenov, B.A.Kim, Jeong-SookKim, Soon-WookKleifges, M.Klimov, P.A.Kreykenbohm, I.Krizmanic, J.F.Królik, K.Kungel, V.Kurihara, Y.Kusenko, A.Kuznetsov, E.Lahmar, H.Lakhdari, F.Licandro, J.Campano, L. LópezMartínez, F. LópezMackovjak, S.Mahdi, M.Mandát, D.Manfrin, M.Marcelli, L.Marcos, J.L.Marszał, W.Martín, Y.Martinez, O.Mase, K.Mastafa, M.Matthews, J.N.Mebarki, N.Medina-Tanco, G.Menshikov, A.Merino, A.Mese, M.Meseguer, J.Meyer, S.S.Mimouni, J.Miyamoto, H.Mizumoto, Y.Monaco, A.de los Ríos, J.A. MoralesNachtman, J.M.Nagataki, S.Naitamor, S.Napolitano, T.Neronov, A.Nomoto, K.Nonaka, T.Ogawa, T.Ogio, S.Ohmori, H.Olinto, A.V.Onel, Y.Osteria, G.Otte, A.N.Pagliaro, A.Painter, W.Panasyuk, M.I.Panico, B.Parizot, E.Park, I.H.Pastircak, B.Paul, T.Pech, M.Pérez-Grande, I.Perfetto, F.Peter, T.Picozza, P.Pindado, S.Piotrowski, L.W.Piraino, S.Plebaniak, Z.Pollini, A.Popescu, E.M.Prevete, R.Prévôt, G.Prieto, H.Przybylak, M.Puehlhofer, G.Putis, M.Reardon, P.Reno, M.H.Reyes, M.Ricci, M.Frías, M.D. RodríguezMatamala, O.F. RomeroRonga, F.Sabau, M.D.Saccá, G.Sagawa, H.Sahnoune, Z.Saito, A.Sakaki, N.Salazar, H.Sánchez, J.L.Balanzar, J.C. SanchezSantangelo, A.Sanz-Andrés, A.Saprykin, O.A.Sarazin, F.Sato, M.Scagliola, A.Schanz, T.Schieler, H.Schovánek, P.Scotti, V.Serra, M.Sharakin, S.A.Shimizu, H.M.Shinozaki, K.Soriano, J.F.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, M.C.Tameda, Y.Tenzer, C.Thomas, S.B.Tibolla, O.Tkachev, L.G.Tomida, T.Tone, N.Toscano, S.Traïche, M.Tsunesada, Y.Tsuno, K.Turriziani, S.Uchihori, Y.Valdés-Galicia, J.F.Vallania, P.Valore, L.Vankova-Kirilova, G.Venters, T.M.Vigorito, C.Villaseñor, L.Vlcek, B.von Ballmoos, P.Vrabel, M.Wada, S.Watanabe, J.Watts, J.Muñoz, R. WeigandWeindl, A.Wiencke, L.Wille, M.Wilms, J.Yamamoto, T.Yang, J.Yano, H.Yashin, I.V.Yonetoku, D.Yoshida, S.Young, R.Zgura, I.S.Zotov, M.Yu.Marchi, A. Zuccaro
Issue Date
Jan-2024
Publisher
Elsevier B.V.
Keywords
Air fluorescence; Cosmic rays (329); Extensive air showers; High-altitude balloons (738); JEM-EUSO
Citation
Astroparticle Physics, v.154
Indexed
SCOPUS
Journal Title
Astroparticle Physics
Volume
154
URI
https://scholarworks.bwise.kr/skku/handle/2021.sw.skku/108732
DOI
10.1016/j.astropartphys.2023.102891
ISSN
0927-6505
1873-2852
Abstract
The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. The plan of this mission of opportunity on a NASA super pressure balloon test flight was to circle the southern hemisphere. The primary scientific goal was to make the first observations of ultra-high-energy cosmic-ray extensive air showers (EASs) by looking down on the atmosphere with an ultraviolet (UV) fluorescence telescope from suborbital altitude (33 km). After 12 days and 4 h aloft, the flight was terminated prematurely in the Pacific Ocean. Before the flight, the instrument was tested extensively in the West Desert of Utah, USA, with UV point sources and lasers. The test results indicated that the instrument had sensitivity to EASs of ⪆3 EeV. Simulations of the telescope system, telescope on time, and realized flight trajectory predicted an observation of about 1 event assuming clear sky conditions. The effects of high clouds were estimated to reduce this value by approximately a factor of 2. A manual search and a machine-learning-based search did not find any EAS signals in these data. Here we review the EUSO-SPB1 instrument and flight and the EAS search. © 2023 The Authors
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