학술논문

Space experiment TUS on board the Lomonosov satellite as pathfinder of JEM-EUSO
Document Type
Original Paper
Author
Adams, Jr., J. H.Ahmad, S.Albert, J. -N.Allard, D.Anchordoqui, L.Andreev, V.Anzalone, A.Arai, Y.Asano, K.Ave Pernas, M.Baragatti, P.Barrillon, P.Batsch, T.Bayer, J.Bechini, R.Belenguer, T.Bellotti, R.Belov, K.Berlind, A. A.Bertaina, M.Biermann, P. L.Biktemerova, S.Blaksley, C.Blanc, N.Błȩcki, J.Blin-Bondil, S.Blümer, J.Bobik, P.Bogomilov, M.Bonamente, M.Briggs, M. S.Briz, S.Bruno, A.Cafagna, F.Campana, D.Capdevielle, J. -N.Caruso, R.Casolino, M.Cassardo, C.Castellinic, G.Catalano, C.Catalano, G.Cellino, A.Chikawa, M.Christl, M. J.Cline, D.Connaughton, V.Conti, L.Cordero, G.Crawford, H. J.Cremonini, R.Csorna, S.Dagoret-Campagne, S.de Castro, A. J.De Donato, C.de la Taille, C.De Santis, C.del Peral, L.Dell’Oro, A.De Simone, N.Di Martino, M.Distratis, G.Dulucq, F.Dupieux, M.Ebersoldt, A.Ebisuzaki, T.Engel, R.Falk, S.Fang, K.Fenu, F.Fernández-Gómez, I.Ferrarese, S.Finco, D.Flamini, M.Fornaro, C.Franceschi, A.Fujimoto, J.Fukushima, M.Galeotti, P.Garipov, G.Geary, J.Gelmini, G.Giraudo, G.Gonchar, M.González Alvarado, C.Gorodetzky, P.Guarino, F.Guzmán, A.Hachisu, Y.Harlov, B.Haungs, A.Hernández Carretero, J.Higashide, K.Ikeda, D.Ikeda, H.Inoue, N.Inoue, S.Insolia, A.Isgrò, F.Itow, Y.Joven, E.Judd, E. G.Jung, A.Kajino, F.Kajino, T.Kaneko, I.Karadzhov, Y.Karczmarczyk, J.Karus, M.Katahira, K.Kawai, K.Kawasaki, Y.Keilhauer, B.Khrenov, B. A.Kim, J. -S.Kim, S. -W.Kim, S. -W.Kleifges, M.Klimov, P. A.Kolev, D.Kreykenbohm, I.Kudela, K.Kurihara, Y.Kusenko, A.Kuznetsov, E.Lacombe, M.Lachaud, C.Lee, J.Licandro, J.Lim, H.López, F.Maccarone, M. C.Mannheim, K.Maravilla, D.Marcelli, L.Marini, A.Martinez, O.Masciantonio, G.Mase, K.Matev, R.Medina-Tanco, G.Mernik, T.Miyamoto, H.Miyazaki, Y.Mizumoto, Y.Modestino, G.Monaco, A.Monnier-Ragaigne, D.Morales de los Ríos, J. A.Moretto, C.Morozenko, V. S.Mot, B.Murakami, T.Murakami, M. NaganoNagata, M.Nagataki, S.Nakamura, T.Napolitano, T.Naumov, D.Nava, R.Neronov, A.Nomoto, K.Nonaka, T.Ogawa, T.Ogio, S.Ohmori, H.Olinto, A. V.Orleański, P.Osteria, G.Panasyuk, M. I.Parizot, E.Park, I. H.Park, H. W.Pastircak, B.Patzak, T.Paul, T.Pennypacker, C.Perez Cano, S.Peter, T.Picozza, P.Pierog, T.Piotrowski, L. W.Piraino, S.Plebaniak, Z.Pollini, A.Prat, P.Prévôt, G.Prieto, H.Putis, M.Reardon, P.Reyes, M.Ricci, M.Rodríguez, I.Rodríguez Frías, M. D.Ronga, F.Roth, M.Rothkaehl, H.Roudil, G.Rusinov, I.Rybczyński, M.Sabau, M. D.Sáez-Cano, G.Sagawa, H.Saito, A.Sakaki, N.Sakata, M.Salazar, H.Sánchez, S.Santangelo, A.Santiago Crúz, L.Sanz Palomino, M.Saprykin, O.Sarazin, F.Sato, H.Sato, M.Schanz, T.Schieler, H.Scotti, V.Segreto, A.Selmane, S.Semikoz, D.Serra, M.Sharakin, S.Shibata, T.Shimizu, H. M.Shinozaki, K.Shirahama, T.Siemieniec-Oziȩbło, G.Silva López, H. H.Sledd, J.Słomińska, K.Sobey, A.Sugiyama, T.Supanitsky, D.Suzuki, M.Szabelska, B.Szabelski, J.Tajima, F.Tajima, N.Tajima, T.Takahashi, Y.Takami, H.Takeda, M.Takizawa, Y.Tenzer, C.Tibolla, O.Tkachev, L.Tokuno, H.Tomida, T.Tone, N.Toscano, S.Trillaud, F.Tsenov, R.Tsunesada, Y.Tsuno, K.Tymieniecka, T.Uchihori, Y.Unger, M.Vaduvescu, O.Valdés-Galicia, J. F.Vallania, P.Valore, L.Vankova, G.Vigorito, C.Villaseñor, L.von Ballmoos, P.Wada, S.Watanabe, J.Watanabe, S.Watts, Jr, J.Weber, M.Weiler, T. J.Wibig, T.Wiencke, L.Wille, M.Wilms, J.Włodarczyk, Z.Yamamoto, T.Yamamoto, Y.Yang, J.Yano, H.Yashin, I. V.Yonetoku, D.Yoshida, K.Yoshida, S.Young, R.Zotov, M. Yu.Zuccaro Marchi, A.The JEM-EUSO Collaboration
Source
Experimental Astronomy: Astrophysical Instrumentation and Methods. November 2015 40(1):315-326
Subject
Air-shower fluorescence telescope
JEM-EUSO
Pathfinder
Language
English
ISSN
0922-6435
1572-9508
Abstract
Space-based detectors for the study of extreme energy cosmic rays (EECR) are being prepared as a promising new method for detecting highest energy cosmic rays. A pioneering space device – the “tracking ultraviolet set-up” (TUS) – is in the last stage of its construction and testing. The TUS detector will collect preliminary data on EECR in the conditions of a space environment, which will be extremely useful for planning the major JEM-EUSO detector operation.