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What do we know about cosmic rays with energies above 5 EeV?
Jonathan Biteau
Cosmic rays begin to reveal their secrets at energies above 5 EeV. Beyond this characteristic energy, known as the spectral "ankle", the arrival-direction data from the Pierre Auge…
Towards a Cosmic-Ray Energy Scale with the Auger Engineering Radio Array
Max Büsken
Radio detection of cosmic-ray (CR) induced extensive air showers with digital antenna arrays is a matured technique by now. At the Pierre Auger Observatory, the Auger Engineering R…
The Cosmological Optical Convergence: Extragalactic Background Light from TeV Gamma Rays
Lucas Gréaux, Jonathan Biteau, Mireia Nievas Rosillo
The intensity of the extragalactic background (EBL), the accumulated optical and infrared emissions since the first stars, is the subject of a decades-long tension in the optical b…
Large-scale cosmic ray anisotropies with 19 years of data from the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Abdul Halim, P. Abreu +355
Results are presented for the measurement of large-scale anisotropies in the arrival directions of ultra-high-energy cosmic rays detected at the Pierre Auger Observatory during 19…
The distribution of ultra-high-energy cosmic rays along the supergalactic plane measured at the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Abdul Halim, P. Abreu +364
Ultra-high-energy cosmic rays are known to be mainly of extragalactic origin, and their propagation is limited by energy losses, so their arrival directions are expected to correla…
Closing the net on transient sources of ultra-high-energy cosmic rays
Sullivan Marafico, Jonathan Biteau, Antonio Condorelli +2
Arrival directions of ultra-high-energy cosmic rays (UHECRs) observed above eV provide evidence of localized excesses that are key to identifying their sources. W…