Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Filevitch, A."'
Autor:
Bertou, X., Allison, P. S., Bonifazi, C., Bauleo, P., Grunfeld, C. M., Aglietta, M., Arneodo, F., Barnhill, D., Beatty, J. J., Busca, N. G., Creusot, A., Dornic, D., Filevitch, A. Etchegoyen. A., Ghia, P. L., Lhenry-Yvon, I., Medina, M. C., Moreno, E., Nitz, D., Ohnuki, T., Ranchon, S., Salazar, H., Suomijärvi, T., Supanitsky, D., Tripathi, A., Urban, M., Villasenor, L.
Publikováno v:
Nucl.Instrum.Meth.A 568 (2006) 839-846
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies ($>10^{19}$ eV). The ground array of the Observatory will consist of 1600 water Cherenkov detectors deployed over 3000 km^2. The remoteness and large number of dete
Externí odkaz:
http://arxiv.org/abs/2102.01656
Autor:
J. J. Beatty, E. Moreno, Humberto Ibarguen Salazar, T. Suomijärvi, C. Grunfeld, M. C. Medina, A. Filevitch, S. Ranchon, A. K. Tripathi, N.G. Busca, P. Bauleo, Marco Aglietta, D. Barnhill, Piera Luisa Ghia, I. Lhenry-Yvon, A. Creusot, Xavier Bertou, A. Etchegoyen, D. Supanitsky, D. Nitz, M. Urban, T. Ohnuki, C. Bonifazi, L. Villaseñor, Patrick Allison, F. Arneodo, D. Dornic
Publikováno v:
Scopus-Elsevier
Web of Science
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2006, 568, pp.839-846. ⟨10.1016/j.nima.2006.07.066⟩
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Web of Science
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Elsevier, 2006, 568, pp.839-846. ⟨10.1016/j.nima.2006.07.066⟩
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies ($>10^{19}$ eV). The ground array of the Observatory will consist of 1600 water Cherenkov detectors deployed over 3000 km^2. The remoteness and large number of dete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::50f9779ee3c3ffbf908c5def2ca92cd9
http://arxiv.org/abs/2102.01656
http://arxiv.org/abs/2102.01656
Autor:
Bertou, X., Allison, P.S., Bonifazi, C., Bauleo, P., Grunfeld, C.M., Aglietta, M., Arneodo, F., Barnhill, D., Beatty, J.J., Busca, N.G., Creusot, A., Dornic, D., Etchegoyen, A., Filevitch, A., Ghia, P.L., Lhenry-Yvon, I., Medina, M.C., Moreno, E., Nitz, D., Ohnuki, T., Ranchon, S., Salazar, H., Suomijärvi, T., Supanitsky, D., Tripathi, A., Urban, M., Villasenor, L.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A 2006 568(2):839-846
Conference
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