Daniela Mockler (Avtor), Andrej Filipčič (Avtor), Gašper Kukec Mezek (Avtor), A. Saleh (Avtor), Samo Stanič (Avtor), M. Trini (Avtor), Serguei Vorobiov (Avtor), Danilo Zavrtanik (Avtor), Marko Zavrtanik (Avtor), Lukas Zehrer (Avtor)

Povzetek

The flux of ultra-high energy cosmic rays above 3×10[sup]17 eV has been measured with unprecedented precision at the Pierre Auger Observatory. The flux of the cosmic rays is determined by four different measurements. The surface detector array provides three data sets, two formed by dividing the data into two zenith angle ranges, and one obtained from a nested, denser detector array. The fourth measurement is obtained with the fluorescence detector. By combining all four data sets, the all-sky flux of cosmic rays is determined. The spectral features are discussed in detail and systematic uncertainties are addressed.

Ključne besede

ultra-high-energy cosmic rays;Pierre Auger Observatory;UHECR energy spectrum;

Podatki

Jezik: Angleški jezik
Leto izida:
Tipologija: 1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija: UNG - Univerza v Novi Gorici
UDK: 539.1
COBISS: 167964163 Povezava se bo odprla v novem oknu
ISSN: 2100-014X
Št. ogledov: 36
Št. prenosov: 0
Ocena: 0 (0 glasov)
Metapodatki: JSON JSON-RDF JSON-LD TURTLE N-TRIPLES XML RDFA MICRODATA DC-XML DC-RDF RDF

Ostali podatki

Vrsta dela (COBISS): Delo ni kategorizirano
Strani: str. 1-4
Letnik: ǂVol. ǂ209
Zvezek: ǂ[article no.] ǂ01029
Čas izdaje: 2019
DOI: 10.1051/epjconf/201920901029
ID: 20176037
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