Astrophysical interpretation of Pierre Auger Observatory measurements of the UHECR energy spectrum and mass composition
We present a combined fit of a simple astrophysical model of UHECR sources to both the energy spectrum and mass composition data measured by the Pierre Auger Observatory. The fit has been performed for energies above 5 EeV, i.e. the region of the all-particle spectrum above the so-called “ankle”’ fe...
Main Author: | di Matteo Armando |
---|---|
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2017-01-01
|
Series: | EPJ Web of Conferences |
Online Access: | https://doi.org/10.1051/epjconf/201713602002 |
Similar Items
-
Studies of the UHECR Mass Composition and Hadronic Interactions with the FD and SD of the Pierre Auger Observatory
by: Carceller J. M.
Published: (2019-01-01) -
Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory
by: Alvarez-Muñiz Jaime
Published: (2019-01-01) -
Fast Radio Bursts and Multimessenger Astrophysics with the Pierre Auger Observatory
by: Maria Alexandra Lima Fernandes
Published: (2021) -
Mass Composition of UHECRs from <i>X</i><sub>max</sub> Distributions Recorded by the Pierre Auger and Telescope Array Observatories
by: Nicusor Arsene
Published: (2021-08-01) -
Measurement of the cosmic ray spectrum with the Pierre Auger Observatory
by: Mockler Daniela
Published: (2019-01-01)