Vladimír Novotný (Author), Andrej Filipčič (Author), J. P. Lundquist (Author), Samo Stanič (Author), Serguei Vorobiov (Author), Danilo Zavrtanik (Author), Marko Zavrtanik (Author), Lukas Zehrer (Author)

Abstract

We present the energy spectrum of cosmic rays measured at the Pierre Auger Observatory from 6×10^15 eV up to the most extreme energies where the accumulated exposure reaches about 80 000 km^2sr yr. The wide energy range is covered with five different measurements, namely using the events detected by the surface detector with zenith angles below 60 degrees and applying different reconstruction method also above 60 degrees, those collected by a denser array, the hybrid events simultaneously recorded by the surface and fluorescence detectors, and using those events in which the signal is dominated by Cherenkov light registered by the high-elevation telescopes. In this contribution, we report updates of the analysis techniques and present the spectrum obtained by combining the five different measurements. Spectral features occurring in the wide energy range covered by the Observatory are discussed.

Keywords

Pierre Auger Observatory;indirect detection;fluorescence detection;surface detection;hybrid detection;ultra-high energy;cosmic rays;cerenkov light;energy spectrum;inclined showers;

Data

Language: English
Year of publishing:
Typology: 1.08 - Published Scientific Conference Contribution
Organization: UNG - University of Nova Gorica
UDC: 539.1
COBISS: 166740995 Link will open in a new window
ISSN: 1824-8039
Views: 22
Downloads: 0
Average score: 0 (0 votes)
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Other data

Type (COBISS): Not categorized
Pages: str. 1-12
Chronology: 2022
DOI: 10.22323/1.395.0324
ID: 20029553