Sub-micron alignment for nuclear emulsion plates using low energy electrons caused by radioactive isotopes

Autor: M. Kazuyama, S. Takahashi, T. Fukuda, S. Miyamoto, Osamu Sato, Masahiro Komatsu, Toshiyuki Nakano, Akitaka Ariga, K. Niwa

Publikováno v: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 575:466-469

Nuclear emulsion plates are employed in three-dimensional charged particle detectors that have sub-micron position resolution over 1 m 2 with no dead space and no dead time. These detectors are suitable for the study of short-lived particle decays, a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::68c51e4afb0ba559b5003c41355181fd
https://doi.org/10.1016/j.nima.2007.02.105

Measurement of the atmospheric muon charge ratio with the OPERA detector

Autor: A. Schembri, T. Matsuo, Ante Ljubičić, Alessandro Paoloni, F. Grianti, T. M. Roganova, Dmitry Golubkov, R. Brugnera, J. Lenkeit, Naotaka Naganawa, F. Juget, Pierre Vilain, N. Mauri, J. Ebert, F. Di Capua, M. Tenti, L. Votano, K. Pretzl, C. Lazzaro, V. Boyarkin, Tomoko Ariga, M. De Serio, Antonio Ereditato, C. Sirignano, F. Dal Corso, Hiroki Rokujo, T. Tran, S. Miyamoto, Akitaka Ariga, M. S. Vladimirov, M. Besnier, André Rubbia, Y. Déclais, B. D. Park, Amina Zghiche, Yu. Zaitsev, A. Garfagnini, Nicola D'Ambrosio, C. Oldorf, Caren Hagner, N. Agafonova, Tatsuhiro Naka, T. Brugière, J. Yoshida, Shigeki Aoki, R. A. Fini, F. Meisel, A. G. Olchevski, I. Kreslo, S. Zemskova, H. Shibuya, D. Duchesneau, F. Pupilli, A. Badertscher, O. Egorov, Satoru Takahashi, E. Medinaceli, G. Brunetti, L. Chaussard, F. Terranova, C. Goellnitz, C. Gustavino, C. Fukushima, S. Dmitrievski, M. Spinetti, R. I. Enikeev, G. Rosa, U. Moser, M. Nakamura, Torben Ferber, G. Romano, P. Migliozzi, Maximiliano Sioli, N. Chon-Sen, Krešimir Jakovčić, A. Cazes, Y. A. Gornushkin, A. Russo, N. G. Polukhina, G. Policastro, Yoshihiro Sato, Cécile Jollet, Luigi Salvatore Esposito, J. Knuesel, G. D'Amato, H. Kubota, M. Giorgini, Anselmo Meregaglia, Guillaume Lutter, N. Di Marco, G. Grella, M. T. Muciaccia, S. Simone, L. A. Goncharova, C. Pistillo, V. G. Ryasny, O. G. Ryazhskaya, Mario Stipčević, M. Cozzi, A. Di Giovanni, G. Felici, Seok Kim, M. Kimura, M. Pozzato, M. Kazuyama, P. A. Publichenko, S. Ogawa, Murat Guler, P. Strolin, H. Pessard, I. G. Park, V. A. Matveev, M. Hierholzer, Kimio Niwa, Koichi Kodama, Marcos Dracos, A. M. Anokhina, V. I. Galkin, W. Schmidt Parzefall, Salvatore Buontempo, A. S. Malgin, S. Tufanli, R. Zimmermann, Toshiyuki Nakano, T. Hara, M. M. Chernyavsky, A. Sheshukov, C. S. Yoon, Dmitry V. Naumov, G. De Lellis, U. Kose, D. Di Ferdinando, M. Ieva, S. Mikado, V. Chiarella, M. Paniccia, R. Rescigno, H. Schroeder, A. V. Bagulya, L. Scotto Lavina, P. Monacelli, D. Frekers, Kunihiro Morishima, Björn Wonsak, D. Autiero, V. I. Osedlo, Gaston Wilquet, P. Tolun, T. Yoshioka, J. Favier, Luca Stanco, E. Pennacchio, J. L. Vuilleumier, Alessandra Pastore, T. Fukuda, V. Nikitina, D. Bick, K. Hamada, A. Bertolin, J. S. Song, Masahiro Komatsu, G. Giacomelli, I. Tezuka, V. F. Yakushev, G. Sirri, Artem Chukanov, Cristiano Bozza, V. Tioukov, A. Marotta, Thomas Strauss, B. Klicek, L. Patrizii, G. Mandrioli, I. Rostovtseva, N. I. Starkov, J. Goldberg, Osamu Sato, G. I. Orlova, S. Dusini, K. Hoshino, V. Pilipenko, Y. Nonoyama, A. Longhin, J. Marteau

Publikováno v: European Physical Journal C. Particles and Fields, 67
European Physical Journal C: Particles and Fields
European Physical Journal C: Particles and Fields, Springer Verlag (Germany), 2010, 67, pp.25-37
Eur.Phys.J.

The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008 CNGS run.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5cdafc045ad3f8ec97b1a563969e7b1b
https://doi.org/10.1140/epjc/s10052-010-1284-8

First events from the CNGS neutrino beam detected in the OPERA experiment

Autor: R Acquafredda, N Agafonova, M Ambrosio, A Anokhina, S Aoki, A Ariga, L Arrabito, D Autiero, A Badertscher, E Baussan, A Bergnoli, F Bersani Greggio, M Besnier, M Beyer, S Bondil-Blin, K Borer, J Boucrot, V Boyarkin, C Bozza, R Brugnera, S Buontempo, Y Caffari, J E Campagne, B Carlus, E Carrara, A Cazes, L Chaussard, M Chernyavsky, V Chiarella, N Chon-Sen, A Chukanov, R Ciesielski, L Consiglio, M Cozzi, F Dal Corso, N D'Ambrosio, J Damet, G De Lellis, Y Déclais, T Descombes, M De Serio, F Di Capua, D Di Ferdinando, A Di Giovanni, N Di Marco, C Di Troia, S Dmitrievski, M Dracos, D Duchesneau, B Dulach, S Dusini, J Ebert, R Enikeev, A Ereditato, L S Esposito, C Fanin, J Favier, G Felici, T Ferber, L Fournier, A Franceschi, D Frekers, T Fukuda, C Fukushima, V I Galkin, V A Galkin, R Gallet, A Garfagnini, G Gaudiot, G Giacomelli, O Giarmana, M Giorgini, L Girard, C Girerd, C Goellnitz, J Goldberg, Y Gornoushkin, G Grella, F Grianti, C Guerin, M Guler, C Gustavino, C Hagner, T Hamane, T Hara, M Hauger, M Hess, K Hoshino, M Ieva, M Incurvati, K Jakovcic, J Janicsko Csathy, B Janutta, C Jollet, F Juget, M Kazuyama, S H Kim, M Kimura, J Knuesel, K Kodama, D Kolev, M Komatsu, U Kose, A Krasnoperov, I Kreslo, Z Krumstein, I Laktineh, C de La Taille, T Le Flour, S Lieunard, A Ljubicic, A Longhin, A Malgin, K Manai, G Mandrioli, U Mantello, A Marotta, J Marteau, G Martin-Chassard, V Matveev, M Messina, L Meyer, S Micanovic, P Migliozzi, S Miyamoto, P Monacelli, I Monteiro, K Morishima, U Moser, M T Muciaccia, P Mugnier, N Naganawa, M Nakamura, T Nakano, T Napolitano, M Natsume, K Niwa, Y Nonoyama, A Nozdrin, S Ogawa, A Olchevski, D Orlandi, D Ossetski, A Paoloni, B D Park, I G Park, A Pastore, L Patrizii, L Pellegrino, H Pessard, V Pilipenko, C Pistillo, N Polukhina, M Pozzato, K Pretzl, P Publichenko, L Raux, J P Repellin, T Roganova, G Romano, G Rosa, A Rubbia, V Ryasny, O Ryazhskaya, D Ryzhikov, A Sadovski, C Sanelli, O Sato, Y Sato, V Saveliev, N Savvinov, G Sazhina, A Schembri, W Schmidt Parzefall, H Schroeder, H U Schütz, L Scotto Lavina, J Sewing, H Shibuya, S Simone, M Sioli, C Sirignano, G Sirri, J S Song, R Spaeti, M Spinetti, L Stanco, N Starkov, M Stipcevic, P Strolin, V Sugonyaev, S Takahashi, V Tereschenko, F Terranova, I Tezuka, V Tioukov, I Tikhomirov, P Tolun, T Toshito, V Tsarev, R Tsenov, U Ugolino, N Ushida, G Van Beek, V Verguilov, P Vilain, L Votano, J L Vuilleumier, T Waelchli, R Waldi, M Weber, G Wilquet, B Wonsak, R Wurth, J Wurtz, V Yakushev, C S Yoon, Y Zaitsev, I Zamboni, R Zimmermann

Publikováno v: New Journal of Physics
New Journal of Physics, Institute of Physics: Open Access Journals, 2006, 8, pp.303. ⟨10.1088/1367-2630/8/12/303⟩

The OPERA neutrino detector at the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in appearance mode, through the study of nu_mu to nu_tau oscillations. The apparatus consists of a lead/e

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::34e6747900d0f1a80abf68b16bc495b3
http://hdl.handle.net/10281/26965

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