✦ LIBER ✦

Calibration of the surface array of the Pierre Auger Observatory

✍ Scribed by X. Bertou; P.S. Allison; C. Bonifazi; P. Bauleo; C.M. Grunfeld; M. Aglietta; F. Arneodo; D. Barnhill; J.J. Beatty; N.G. Busca; A. Creusot; D. Dornic; A. Etchegoyen; A. Filevitch; P.L. Ghia; I. Lhenry-Yvon; M.C. Medina; E. Moreno; D. Nitz; T. Ohnuki; S. Ranchon; H. Salazar; T. Suomijärvi; D. Supanitsky; A. Tripathi; M. Urban; L. Villasenor

Publisher: Elsevier Science
Year: 2006
Tongue: English
Weight: 426 KB
Volume: 568
Category: Article
ISSN: 0168-9002
DOI: 10.1016/j.nima.2006.07.066

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Trigger and aperture of the surface dete

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

✍ J. Abraham; P. Abreu; M. Aglietta; E.J. Ahn; D. Allard; I. Allekotte; J. Allen; 📂 Article 📅 2010 🏛 Elsevier Science 🌐 English ⚖ 591 KB

The Surface Detector of the Pierre Auger

The Surface Detector of the Pierre Auger Observatory

✍ Jan Ridky 📂 Article 📅 2007 🏛 Elsevier Science 🌐 English ⚖ 312 KB

Operation of the Pierre Auger Observator

Operation of the Pierre Auger Observatory

✍ Julio Rodriguez Martino 📂 Article 📅 2011 🏛 Elsevier Science 🌐 English ⚖ 502 KB

Multi-wavelength calibration procedure f

Multi-wavelength calibration procedure for the pierre Auger Observatory Fluorescence Detectors

✍ A.C. Rovero; P. Bauleo; J.T. Brack; J.L. Harton; R. Knapik 📂 Article 📅 2009 🏛 Elsevier Science 🌐 English ⚖ 830 KB

Status of the Southern Pierre Auger Obse

Status of the Southern Pierre Auger Observatory

✍ M. Kleifges 📂 Article 📅 2006 🏛 Elsevier Science 🌐 English ⚖ 840 KB

Enhancing the Pierre Auger Observatory t

Enhancing the Pierre Auger Observatory to the – eV range: Capabilities of an Infill Surface Array

✍ M.C. Medina; M. Gómez Berisso; I. Allekotte; A. Etchegoyen; G. Medina Tanco; A.D 📂 Article 📅 2006 🏛 Elsevier Science 🌐 English ⚖ 271 KB

The Pierre Auger Observatory has been designed to study the highest-energy cosmic rays in nature (EX10 18:5 eV). The determination of their arrival direction, energy and composition is performed by the analysis of the atmospheric showers they produce. The Auger Surface Array will consist of 1600 wat