作者
J Abraham, M Aglietta, IC Aguirre, M Albrow, D Allard, I Allekotte, P Allison, J Alvarez Muniz, MG Do Amaral, M Ambrosio, L Anchordoqui, R Andrews, M Anguiano, JC Dos Anjos, C Aramo, Stefano Argiro, K Arisaka, JC Arteaga, S Atulugama, M Ave, G Avila, R Baggio, X Bai, AF Barbosa, HMJ Barbosa, D Barnhill, SLC Barroso, P Bauleo, J Beatty, T Beau, K-H Becker, JA Bellido, P Bello, T Bergmann, E Berman, X Bertou, P Biermann, P Billoir, R Biral, H Bluemer, M Bohacova, E Bollmann, C Bonifazi, M Boratav, A Boselli, J Brack, J-M Brunet, H Bui-Duc, V Cabrera, DV Camin, J-N Capdevielle, A Carreño, N Cartiglia, R Caruso, LA De Carvalho, S Casanova, E Casimiro, A Castellina, J Castro, PW Cattaneo, L Cazon, R Cester, N Chavez, D Cheam, A Chiavassa, JA Chinellato, M Chiosso, A Chou, J Chye, A Cillis, B Civit, D Claes, PDJ Clark, RW Clay, F Cohen, A Cordero, A Cordier, E Cormier, J Cotzomi, U Cotti, S Coutu, CE Covault, A Creusot, JW Cronin, M Cuautle, S Dagoret-Campagne, T Dang-Quang, P Da Silva, J Darling, P Darriulat, K Daumiller, BR Dawson, L De Bruijn, A De Capoa, MAL De Oliveira, V De Souza, A Della Selva, O Deligny, JC Diaz, C Dobrigkeit, JC D'Olivo, A Dorofeev, MT Dova, A Dye, MA DuVernois, R Engel, LN Epele, P Eschstruth, CO Escobar, A Etchegoyen, P Facal San Luis, AC Fauth, N Fazzini, Arnaud Fernandez, AMJ Ferrero, B Fick, A Filevich, A Filipčič, R Fonte, W Fulgione, E Gamez, B Garcia, CA Garcia, H Geenen, H Gemmeke, C Germain-Renaud, PL Ghia, K Gibbs, M Giller, J Gitto, H Glass, M Gómez Berisso, PF Gomez Vitale, J Gonzalez, D Gora, A Goodwin, P Gouffon, V Grassi, AF Grillo, C Grunfeld, J Grygar, F Guarino, G Guedes, C Guerard, R Gumbsheimer, JL Harton, F Hasenbalg, D Heck, JM Hernandez, D Hoffer
发表日期
2004/5/1
期刊
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
卷号
523
期号
1-2
页码范围
50-95
出版商
North-Holland
简介
Construction of the first stage of the Pierre Auger Observatory has begun. The aim of the Observatory is to collect unprecedented information about cosmic rays above 10 18eV . The first phase of the project, the construction and operation of a prototype system, known as the engineering array, has now been completed. It has allowed all of the sub-systems that will be used in the full instrument to be tested under field conditions. In this paper, the properties and performance of these sub-systems are described and their success illustrated with descriptions of some of the events recorded thus far.
引用总数
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J Abraham, M Aglietta, IC Aguirre, M Albrow, D Allard… - Nuclear Instruments and Methods in Physics Research …, 2004