4.4 Article

Trigger and aperture of the surface detector array of the Pierre Auger Observatory

出版社

ELSEVIER
DOI: 10.1016/j.nima.2009.11.018

关键词

Ultra high energy cosmic rays; Auger Observatory; Extensive air showers; Trigger; Exposure

资金

  1. Comision Nacional de Energia Atomica
  2. Fundacion Antorchas
  3. Gobierno De La Provincia de Mendoza
  4. Municipalidad de Malargue
  5. NDM Holdings
  6. Valle Las Lenas
  7. Australian Research Council
  8. Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)
  9. Financiadora de Estudos e Projetos (FINEP)
  10. Fundacao de Amparo A Pesquisa do Estado de Rio de Janeiro (FAPERJ)
  11. Fundacao de Amparo Pesquisa do Estado de Sao Paulo (FAPESP)
  12. Ministerio de Ciencia e Tecnologia (MCT), Brazil [AVOZ10100502, AV0Z101100522, GAAV KJB300100801, KJB100100904, MSMT-CR LA08016, LC527, 1M06002, MSM0021620859,]
  13. Czech Republic
  14. Centre de Calcul [IN2P3/CNRS]
  15. Centre National de la Recherche Scientifique (CNRS)
  16. Conseil Regional Ile-de-France
  17. Departement Physique Nucleaire et Corpusculaire [PNC-IN2P3/CNRS]
  18. Departement Sciences de I'Univers (SDU-INSU/CNRS), France
  19. Bundesministerium fur Bildung und Forschung (BMBF)
  20. Deutsche Forschungsgemeinschaft (DFG)
  21. Finanzministerium Baden-Wurttemberg
  22. Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
  23. Ministerium fur Wissenschaft und Forschung
  24. Nordrhein-Westfalen
  25. Ministerium fur Wissenschaft
  26. Forschung und Kunst
  27. Baden-Wurttemberg, Germany
  28. Istituto Nazionale di Fisica Nucleare (INFN)
  29. Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy
  30. Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico
  31. Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
  32. Fundamenteel Onderzoek der Materie (FOM), Netherlands
  33. Ministry of Science and Higher Education [1 P03 D 014 30, N202 090 31/0623, PAP/218/2006]
  34. Fundacao para a Ciencia e a Tecnologia, Portugal
  35. Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia
  36. Consejeria de Educacion de la Comunidad de Castilla La Mancha
  37. FEDER funds
  38. Ministerio de Ciencia e Innovacion
  39. Xunta de Galicia, Spain
  40. Science and Technology Facilities Council, UK: Department of Energy [DE-AC02-07CH11359]
  41. National Science Foundation [0450696]
  42. Grainger Foundation USA
  43. ALFA-EC / HELEN
  44. European Union [MEIF-CT-2005-025057, PIEF-GA-2008-220240]
  45. UNESCO
  46. Division Of Physics
  47. Direct For Mathematical & Physical Scien [0838088] Funding Source: National Science Foundation
  48. Science and Technology Facilities Council [PP/E007007/1] Funding Source: researchfish
  49. STFC [PP/E007007/1] Funding Source: UKRI

向作者/读者索取更多资源

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive air showers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the identification of candidate showers at the level of a single detector, amongst a large background (mainly random single cosmic ray muons), up to the selection of real events and the rejection of random coincidences. Such trigger makes the surface detector array fully efficient for the detection of EAS with energy above 3 x 10(18) eV, for all zenith angles between 0 degrees and 60 degrees, independently of the position of the impact point and of the mass of the primary particle. In these range of energies and angles, the exposure of the surface array can be determined purely on the basis of the geometrical acceptance. (C) 2009 Elsevier B.V. All rights reserved.

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