Properties and performance of the prototype instrument for the Pierre Auger Observatory
| dc.contributor.author | Abraham, J. | |
| dc.contributor.author | Aglietta, M. | |
| dc.contributor.author | Aguirre, I. C. | |
| dc.contributor.author | Albrow, M. | |
| dc.contributor.author | Allard, D. | |
| dc.contributor.author | Allekotte, I. | |
| dc.contributor.author | Allison, P. | |
| dc.contributor.author | Alvarez Muñiz, J. | |
| dc.contributor.author | do Amaral, M. G. | |
| dc.contributor.author | Ambrosio, M. | |
| dc.contributor.author | Anchordoqui, L. | |
| dc.contributor.author | Andrews, R. | |
| dc.contributor.author | Anguiano, M. | |
| dc.contributor.author | dos Anjos, J. C. | |
| dc.contributor.author | Aramo, C. | |
| dc.contributor.author | Argiro, S. | |
| dc.contributor.author | Arisaka, K. | |
| dc.contributor.author | Arteaga, J. C. | |
| dc.contributor.author | Atulugama, S. | |
| dc.contributor.author | Ave, M. | |
| dc.contributor.author | Avila, G. | |
| dc.contributor.author | Baggio, R. | |
| dc.contributor.author | Bai, X. | |
| dc.contributor.author | Barbosa, A. F. | |
| dc.contributor.author | Barbosa, H. M. J. | |
| dc.contributor.author | Barnhill, D. | |
| dc.contributor.author | Barroso, S. L. C. | |
| dc.contributor.author | Bauleo, P. | |
| dc.contributor.author | Beatty, J. | |
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| dc.contributor.author | Caruso, R. | |
| dc.contributor.author | de Carvalho, L. A. | |
| dc.contributor.author | Casanova, S. | |
| dc.contributor.author | Casimiro, E. | |
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| dc.contributor.author | Zavrtanik, D. | |
| dc.contributor.author | Zavrtanik, M. | |
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| dc.date.accessioned | 2024-06-28T18:10:20Z | |
| dc.date.available | 2024-06-28T18:10:20Z | |
| dc.date.issued | 2004-05-01 | |
| dc.description.abstract | 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 10¹⁸eV. 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. | |
| dc.description.sponsorship | We are very grateful to the following agencies and organisations for financial support: Gobierno de Mendoza, Comisión Nacional de Energı́a Atómica y Municipalidad de Malargüe, Argentina; the Australian Research Council; Fundacao de Amparo a Pesquisa do Estado de Sao Paulo, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico and Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro, Brasil; National Science Foundation of China, Ministry of Education of the Czech Republic (projects LA134 and LN00A006); Centre National de la Recherche Scientifique, Institut National de Physique Nucléaire et Physique des Particules (IN2P3/CNRS), Institut National des Sciences de l'Univers (INSU/CNRS) et Conseil Régional Ile de France, France; German Ministry for Education and Research and Forschungszentrum Karlsruhe, Germany; Istituto Nazionale di Fisica Nucleare, Italy; Consejo Nacional de Ciencia y Tecnologia, Mexico; the Polish State Committee for Scientific Research (grant numbers PBZ KBN 054/P03/2001, 2 PO3B 110 24 and 2 PO3D 011 24); Ministry of Education, Science and Sport of the Republic of Slovenia; MCyT (grant FPA 2001-3837) and Xunta de Galicia (grant PGIDIT02 PXIC 20611PN), Spain; Particle Physics and Astronomy Research Council, UK, the University of Chicago, the US Department of Energy the US National Science Foundation, USA, and UNESCO. | |
| dc.description.uri | https://www.sciencedirect.com/science/article/pii/S0168900203033497 | |
| dc.format.extent | 46 pages | |
| dc.genre | journal articles | |
| dc.identifier | doi:10.13016/m2hnhb-rmxl | |
| dc.identifier.citation | Abraham, J., M. Aglietta, I. C. Aguirre, M. Albrow, D. Allard, I. Allekotte, P. Allison, et al. “Properties and Performance of the Prototype Instrument for the Pierre Auger Observatory.” Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 523, no. 1 (May 1, 2004): 50–95. https://doi.org/10.1016/j.nima.2003.12.012. | |
| dc.identifier.uri | https://doi.org/10.1016/j.nima.2003.12.012 | |
| dc.identifier.uri | http://hdl.handle.net/11603/34805 | |
| dc.language.iso | en_US | |
| dc.publisher | ELSEVIER | |
| dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
| dc.relation.ispartof | UMBC Physics Department | |
| dc.rights | This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law. | |
| dc.rights | Public Domain | |
| dc.rights.uri | https://creativecommons.org/publicdomain/mark/1.0/ | |
| dc.subject | Extensive air showers | |
| dc.subject | Auger Observatory | |
| dc.subject | Ultra high energy cosmic rays | |
| dc.title | Properties and performance of the prototype instrument for the Pierre Auger Observatory | |
| dc.type | Text | |
| dcterms.creator | https://orcid.org/0000-0002-4027-1855 |
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