Measurement of the cosmic ray energy spectrum using hybrid events of the Pierre Auger Observatory
Data(s) |
01/08/2012
|
---|---|
Resumo |
The energy spectrum of ultra-high energy cosmic rays above 10(18)eV is measured using the hybrid events collected by the Pierre Auger Observatory between November 2005 and September 2010. The large exposure of the Observatory allows the measurement of the main features of the energy spectrum with high statistics. Full Monte Carlo simulations of the extensive air showers (based on the CORSIKA code) and of the hybrid detector response are adopted here as an independent cross check of the standard analysis (Phys. Lett. B 685, 239 (2010)). The dependence on mass composition and other systematic uncertainties are discussed in detail and, in the full Monte Carlo approach, a region of confidence for flux measurements is defined when all the uncertainties are taken into account. An update is also reported of the energy spectrum obtained by combining the hybrid spectrum and that measured using the surface detector array. |
Formato |
application/pdf |
Identificador | |
Idioma(s) |
en |
Publicador |
Springer Heidelberg |
Relação |
http://eprints.ucm.es/38074/ http://dx.doi.org/10.1140/epjp/i2012-12087-9 10.1140/epjp/i2012-12087-9 info:eu-repo/grantAgreement/EC/FP7/246806 LA08016 MEB111003 LG11044 MSM0021620859 LA08015 TA01010517 PNC-IN2P3/CNRS N N202 200239 N N202 207238 DE-AC02-07CH11359 DE-FR02-04ER41300 |
Direitos |
info:eu-repo/semantics/openAccess |
Palavras-Chave | #Física nuclear |
Tipo |
info:eu-repo/semantics/article PeerReviewed |