Cosmogenic photon fluxes at ultra-high energies
Marcus Niechciol, Chiara Jane Papior, Markus Risse
astro-ph.HE
Submitted: 2026-07-16
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Searches for Ultra-High-Energy Photons at the Pierre Auger Observatory
- Production and propagation of ultra-high energy photons using CRPropa 3
- Upper limit on the diffuse extragalactic radio background from GZK photon observation
- CRPropa 3.2 -- an advanced framework for high-energy particle propagation in extragalactic and galactic spaces
- Semi-analytic modeling of the EBL and consequences for extragalactic gamma-ray spectra
- The energy spectrum of cosmic rays beyond the turn-down around $10^{17}$ eV as measured with the surface detector of the Pierre Auger Observatory
- A new view of UHECRs with the Pierre Auger Observatory
- Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory
- Constraining the sources of ultra-high-energy cosmic rays across and above the ankle with the spectrum and composition data measured at the Pierre Auger Observatory
- Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory
- An updated estimate of the cosmic radio background and implications for ultra-high-energy photon propagation
- Search for photons above 10$^{18}$ eV by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory
- AugerPrime: Status and first results
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