Energy spectrum of cosmic rays measured using the Pierre Auger Observatory

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00564862" target="_blank" >RIV/68378271:_____/22:00564862 - isvavai.cz</a>
Alternative codes found
RIV/61989592:15310/22:73616936
Result on the web
<a href="https://pos.sissa.it/395/324/pdf" target="_blank" >https://pos.sissa.it/395/324/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.395.0324" target="_blank" >10.22323/1.395.0324</a>

Result language
angličtina
Original language name
Energy spectrum of cosmic rays measured using the Pierre Auger Observatory
Original language description
We present the energy spectrum of cosmic rays measured at the Pierre Auger Observatory from 6×1015 eV up to the most extreme energies where the accumulated exposure reaches about 80 000 km2sr 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.
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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