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Performances of JEM-EUSO: energy and X (max) reconstruction

Title
Performances of JEM-EUSO: energy and X (max) reconstruction
Authors
Guzman, A.Hachisu, Y.Harlov, B.Haungs, A.Hernandez Carretero, J.Higashide, K.Ikeda, D.Ikeda, H.Inoue, N.Inoue, S.Insolia, A.Isgro, 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, Jeong-SookKim, Soon-WookKim, Sug-WhanKleifges, 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.Lopez, F.Maccarone, M. C.Mannheim, K.Maravilla, D.Marcelli, L.Marini, A.Martinez, O.Masciantonio, G.Mase, K.Ogawa, T.Ogio, S.Matev, R.Medina-Tanco, G.Mernik, T.Miyamoto, H.Miyazaki, Y.Mizumoto, Y.Modestino, G.Monaco, A.Monnier-Ragaigne, D.Morales de Los Rios, J. A.Moretto, C.Morozenko, V. S.Mot, B.Murakami, T.Nagano, M.Nagata, M.Nagataki, S.Nakamura, T.Napolitano, T.Naumov, D.Nava, R.Neronov, A.Nomoto, K.Nonaka, T.Ohmori, H.Olinto, A. V.Orleanski, 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.Prevot, G.Prieto, H.Putis, M.Reardon, P.Reyes, M.Ricci, M.Rodriguez, I.Rodriguez Frias, M. D.Ronga, F.Roth, M.Rothkaehl, H.Roudil, G.Rusinov, I.Rybczynski, M.Sabau, M. D.Saez Cano, G.Sagawa, H.Saito, A.Sakaki, N.Sakata, M.Salazar, H.Sanchez, S.Santangelo, A.Santiago Cruz, 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-Ozieblo, G.Silva Lopez, H. H.Sledd, J.Slominska, 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.Valdes-Galicia, J. F.Vallania, P.Valore, L.Vankova, G.Vigorito, C.Villasenor, L.von Ballmoos, P.Wada, S.Watanabe, J.Watanabe, S.Watts, J., Jr.Weber, M.Weiler, T. J.Wibig, T.Wiencke, L.Wille, M.Wilms, J.Wlodarczyk, Z.Yamamoto, T.Yamamoto, Y.Yang, J.Yano, H.Yashin, I. V.Yonetoku, D.Yoshida, K.Yoshida, S.Young, R.Zotov, M. Yu.JEM-EUSO CollaborationArai, Y.Asano, K.Ave Pernas, M.Adams, J. H., Jr.Ahmad, S.Albert, J. -N.Allard, D.Anchordoqui, L.Andreev, V.Anzalone, A.Baragatti, P.Barrillon, P.Batsch, T.Catalano, O.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.Bayer, J.Bechini, R.Belenguer, T.Bellotti, R.Belov, K.Berlind, A. A.Bertaina, M.Biermann, P. L.Biktemerova, S.Blaksley, C.Blanc, N.Blecki, J.Blin-Bondil, S.Bluemer, 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.Castellini, G.Catalano, C.Ebersoldt, A.Ebisuzaki, T.Engel, R.Falk, S.Fang, K.Fenu, F.Fernandez-Gomez, 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.Gonzalez Alvarado, C.Gorodetzky, P.Guarino, F.
Ewha Authors
양종만
SCOPUS Author ID
양종만scopus
Issue Date
2015
Journal Title
EXPERIMENTAL ASTRONOMY
ISSN
0922-6435JCR Link

1572-9508JCR Link
Citation
EXPERIMENTAL ASTRONOMY vol. 40, no. 1, pp. 183 - 214
Keywords
JEM-EUSOEnergy reconstructionX-max reconstruction
Publisher
SPRINGER
Indexed
SCIE; SCOPUS WOS scopus
Document Type
Article
Abstract
The Extreme Universe Space Observatory (EUSO) on-board the Japanese Experimental Module (JEM) of the International Space Station aims at the detection of ultra high energy cosmic rays from space. The mission consists of a UV telescope which will detect the fluorescence light emitted by cosmic ray showers in the atmosphere. The mission, currently developed by a large international collaboration, is designed to be launched within this decade. In this article, we present the reconstruction of the energy of the observed events and we also address the X (max) reconstruction. After discussing the algorithms developed for the energy and X (max) reconstruction, we present several estimates of the energy resolution, as a function of the incident angle, and energy of the event. Similarly, estimates of the X (max) resolution for various conditions are presented.
DOI
10.1007/s10686-014-9427-9
Appears in Collections:
자연과학대학 > 물리학전공 > Journal papers
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