Accès ouvert
2026
preprint
OpenAlex
T K ND TPC collaboration, A. Abdul Halim, P. Abreu, M. Aglietta et autres
Hybrid measurements at the Pierre Auger Observatory indicate that most high-energy hadronic interaction models underestimate the average depth of the shower maximum, $\langle X_{\max} \rangle$, at a center-of-mass energy of $\sqrt{s}=97.7 \pm 0.4^{+6.6}_{-6.2}\,\mathrm{TeV}$. In this Letter, the hadronic interaction models are shown …
Accès ouvert
2025
preprint
OpenAlex
T K ND TPC collaboration, A. Abdul Halim, P. Abreu, M. Aglietta et autres
Diffuse photons of energy above 0.1 PeV, produced through the interactions between cosmic rays and either interstellar matter or background radiation fields, are powerful tracers of the distribution of cosmic rays in the Galaxy. Furthermore, the measurement of a diffuse photon flux …
fr
(code pays fourni par la source)
Accès ouvert
2025
preprint
OpenAlex
A. Abdul Halim, P. Abreu, M. Aglietta, I. Allekotte et autres
The energy spectrum of cosmic rays above 2.5 EeV has been measured across the declination range $-90^\circ \leqδ\leq +44.8^\circ$ using data from $\sim 310{,}000$ events accrued at the Pierre Auger Observatory from an exposure of $(104{,}900\pm 3{,}100)$ km$^2\,$sr$\,$yr. No significant variations of …
fr
(code pays fourni par la source)
2023
article
OpenAlex
Pedro Abreu, Marco Aglietta, Gioacchino Alex Anastasi, Luis Miguel Domingues Mendes et autres
Accès ouvert
2021
preprint
OpenAlex
T K ND TPC collaboration, P. Abreu, M. Aglietta, J M Albury et autres
Lorentz invariance violation (LIV) is often described by dispersion relations of the form $E_i^2=m_i^2+p_i^2+δ_{i,n} E^{2+n}$ with delta different based on particle type $i$, with energy $E$, momentum $p$ and rest mass $m$. Kinematics and energy thresholds of interactions are modified once the …
fr
(code pays fourni par la source)
Accès ouvert
2020
article
OpenAlex
T K ND TPC collaboration, A. Aab, P. Abreu, M. Aglietta et autres
To obtain direct measurements of the muon content of extensive air showers with energy above $10^{16.5}$ eV, the Pierre Auger Observatory is currently being equipped with an underground muon detector (UMD), consisting of 219 10 $\mathrm{m^2}$-modules, each segmented into 64 scintillators coupled …
nl, pt, it, au, ar, es, us, de, mx, ro, cz, pe, fr, br, pl, be
(code pays fourni par la source)
Accès ouvert
2020
article
OpenAlex
T K ND TPC collaboration, A. Aab, P. Abreu, M. Aglietta et autres
Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the …
nl, pt, it, au, ar, mx, es, us, de, ro, cz, fr, br, pl, be
(code pays fourni par la source)
Accès ouvert
2020
article
OpenAlex
Alexander Aab, Pedro Abreu, Belén Andrada, Martin Erdmann et autres
Accès ouvert
2015
preprint
OpenAlex
IceCube Collaboration, M. G. Aartsen, K. Abraham, M. Ackermann et autres
We have conducted three searches for correlations between ultra-high energy cosmic rays detected by the Telescope Array and the Pierre Auger Observatory, and high-energy neutrino candidate events from IceCube. Two cross-correlation analyses with UHECRs are done: one with 39 cascades from the …
Accès ouvert
2015
article
OpenAlex
A. Aab, P. Abreu, M. Aglietta, E.J. Ahn et autres
Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E > = 6×1019 eV by analyzing cosmic rays with energies above E …
2013
article
OpenAlex
[No Value] The Pierre Auger Collaboration, A. Aab, Pedro Abreu, Marco Aglietta et autres
2013
conference-paper
OpenAlex
The Telescope Array Collaboration, Diego Torres Machado, G. C. Hill, P. Necesal et autres
Joint contributions of the Pierre Auger and Telescope Array Collaborations to the 33rd International Cosmic Ray Conference, Rio de Janeiro, Brazil, July 2013: cross-calibration of the fluorescence telescopes, large scale anisotropies and mass composition.