The CALOCUBE project for a space based cosmic ray experiment: design, construction, and first performance of a high granularity calorimeter prototype

Autor: O., Adriani, S., Albergo, L., Auditore, A., Basti, E., Berti, G., Bigongiari, L., Bonechi, M., Bongi, V., Bonvicini, S., Bottai, P., Brogi, G., Cappello, G., Carotenuto, G., Castellini, W., Cattaneo P., R., Cecchi, C., Checchia, R., D'Alessandro, S., Detti, M., Fasoli, N., Finetti, A., Italiano, P., Lenzi, P., Maestro, M., Manetti, S., Marrocchesi P., N., Mori, F., Morsani, M., Olmi, A., Orsini, G., Orzan, L., Pacini, P., Papini, G., Pellegriti M., A., Rappoldi, S., Ricciarini, A., Sciuto, P., Spillantini, O., Starodubtsev, L., Stiaccini, F., Stolzi, A., Sulaj, E., Suh J., A., Tiberio, A., Tricomi, A., Trifiro, M., Trimarchi, E., Vannuccini, A., Vedda, Zampa, G., N, N. Zampa

Current research in High Energy Cosmic Ray Physics touches on fundamental questions regarding the origin of cosmic rays, their composition, the acceleration mechanisms, and their production. Unambiguous measurements of the energy spectra and of the c

Externí odkaz: http://arxiv.org/abs/1910.09784

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CALET Search for electromagnetic counterparts of gravitational waves during the LIGO/Virgo O3 run

Autor: O. Adriani, Y. Akaike, K. Asano, Y. Asaoka, E. Berti, G. Bigongiari, W. R. Binns, M. Bongi, P. Brogi, A. Bruno, J. H. Buckley, N. Cannady, G. Castellini, C. Checchia, M. L. Cherry, G. Collazuol, K. Ebisawa, A. W. Ficklin, H. Fuke, S. Gonzi, T. G. Guzik, T. Hams, K. Hibino, M. Ichimura, K. Ioka, W. Ishizaki, M. H. Israel, K. Kasahara, J. Kataoka, R. Kataoka, Y. Katayose, C. Kato, N. Kawanaka, Y. Kawakubo, K. Kobayashi, K. Kohri, H. S. Krawczynski, J. F. Krizmanic, P. Maestro, P. S. Marrocchesi, A. M. Messineo, J. W. Mitchell, S. Miyake, A. A. Moiseev, M. Mori, N. Mori, H. M. Motz, K. Munakata, S. Nakahira, J. Nishimura, G. A. de Nolfo, S. Okuno, J. F. Ormes, N. Ospina, S. Ozawa, L. Pacini, P. Papini, B. F. Rauch, S. B. Ricciarini, K. Sakai, T. Sakamoto, M. Sasaki, Y. Shimizu, A. Shiomi, P. Spillantini, F. Stolzi, S. Sugita, A. Sulaj, M. Takita, T. Tamura, T. Terasawa, S. Torii, Y. Tsunesada, Y. Uchihori, E. Vannuccini, J. P. Wefel, K. Yamaoka, S. Yanagita, A. Yoshida, K. Yoshida, W. V. Zober

The CALorimetric Electron Telescope (CALET) on the International Space Station (ISS) consists of a high-energy cosmic ray CALorimeter (CAL) and a lower-energy CALET Gamma ray Burst Monitor (CGBM). CAL is sensitive to electrons up to 20 TeV, cosmic ra

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6cd158946a7c6edc85cc57994742a4c4
http://arxiv.org/abs/2207.03621

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Investigating the Vela SNR's Emission of Electron Cosmic Rays with CALET at the International Space Station

Autor: John F. Krizmanic, A. Sulaj, S. Miyake, P. Spillantini, Holger Motz, Y. Katayose, M. Takita, S. Sugita, Ryuho Kataoka, K. Kobayashi, W.V. Zober, O. Adriani, K. Ebisawa, Y. Tsunesada, Gabriele Bigongiari, Kazutaka Yamaoka, Kunihito Ioka, Eugenio Berti, A. Yoshida, J. P. Wefel, L. Pacini, J. F. Ormes, Michael Cherry, T. Sakamoto, A. A. Moiseev, M. Ichimura, Jason Link, Shoji Torii, A.W. Ficklin, Jun Kataoka, Yoichi Asaoka, Masaki Mori, Katsuaki Asano, Thomas Hams, S. Ozawa, P. S. Marrocchesi, John Mitchell, Jun Nishimura, Sandro Gonzi, Y. Akaike, M. H. Israel, F. Stolzi, Henric Krawczynski, Y. Shimizu, N. Ospina, H. Fuke, Paolo Brogi, K. Sakai, Chihiro Kato, Kazunori Kohri, M. Bongi, S. Okuno, A. Shiomi, N. Mori, Y. Uchihori, N. Cannady, K. Hibino, W. R. Binns, T. Tamura, M. Sasaki, G. Castellini, G. Collazuol, K. Kasahara, T. G. Guzik, J. H. Buckley, Shohei Yanagita, Satoshi Nakahira, Y. Kawakubo, A. Bruno, W. Ishizaki, Alberto Messineo, C. Checchia, S. B. Ricciarini, Kazuoki Munakata, P. Papini, E. Vannuccini, Toshio Terasawa, Kenji Yoshida, Paolo Maestro, G. A. de Nolfo, Norita Kawanaka, Brian Rauch

Publikováno v: Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).

The ISS-based Calorimetric Electron Telescope (CALET) is directly measuring the energy spec- trum of electron+positron cosmic rays up to 20 TeV. Cosmic-ray electrons of TeV region energy are limited by energy loss to a propagation range of about 1 kp

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::bfdd7fe5adbc8a5646657c080b5a139f
https://doi.org/10.22323/1.395.0100