Energy spectrum of cosmic rays measured using the Pierre Auger Observatory

Kód výsledku v 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>

Nalezeny alternativní kódy

RIV/61989592:15310/22:73616936

Výsledek na webu

<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>

Jazyk výsledku

angličtina

Název v původním jazyce

Energy spectrum of cosmic rays measured using the Pierre Auger Observatory

Popis výsledku v původním jazyce

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.

Název v anglickém jazyce

Energy spectrum of cosmic rays measured using the Pierre Auger Observatory

Popis výsledku anglicky

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.

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2022

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název statě ve sborníku

Proceedings of Science

ISBN

—

ISSN

1824-8039

e-ISSN

—

Počet stran výsledku

12

Strana od-do

324

Název nakladatele

Sissa Medilab srl

Místo vydání

Trieste

Místo konání akce

Berlin

Datum konání akce

12. 7. 2021

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

—