A search for photons with energies above eV using hybrid data from the low-energy extensions of the Pierre Auger Observatory
arXiv:2205.14864 · doi:10.3847/1538-4357/ac7393
Abstract
Ultra-high-energy photons with energies exceeding eV offer a wealth of connections to different aspects of cosmic-ray astrophysics as well as to gamma-ray and neutrino astronomy. The recent observations of photons with energies in the eV range further motivate searches for even higher-energy photons. In this paper, we present a search for photons with energies exceeding eV using about 5.5 years of hybrid data from the low-energy extensions of the Pierre Auger Observatory. The upper limits on the integral photon flux derived here are the most stringent ones to date in the energy region between and eV.
Accepted for publication in ApJ
References in corpus (15)
- Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
- First Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies
- The Offline Software Framework of the Pierre Auger Observatory
- Gravitational Production of Dark Matter during Reheating
- The energy spectrum of cosmic rays beyond the turn-down around eV as measured with the surface detector of the Pierre Auger Observatory
- Search for ultra-high energy photons using air showers
- AugerPrime: the Pierre Auger Observatory Upgrade
- Radiative Production of Non-thermal Dark Matter
- KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV
- Evidence of 200 TeV photons from HAWC J1825-134
- Discovery of the Ultra-high energy gamma-ray source LHAASO J2108+5157
- Hunting for super-heavy dark matter with the highest-energy cosmic rays
- Hunting super-heavy dark matter with ultra-high energy photons
- Characteristics of geomagnetic cascading of ultra-high energy photons at the southern and northern sites of the Pierre Auger Observatory
- Diffuse flux of ultra-high energy photons from cosmic-ray interactions in the disk of the Galaxy and implications for the search for decaying super-heavy dark matter
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- Combined Fit of Spectrum and Composition for FR0 Radio-galaxy-emitted Ultra-high-energy Cosmic Rays with Resulting Secondary Photons and Neutrinos
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