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UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby galaxies
- 1.0564975 - FZÚ 2023 RIV IT eng C - Conference Paper (international conference)
Abreu, A. - Aglietta, M. - Albury, J.M. - Bakalová, Alena - Blažek, Jiří - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Hamal, Petr - Janeček, Petr - Juryšek, Jakub - Mandát, Dušan - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Řídký, Jan - dos Santos, Eva M. Martins - Schovánek, Petr - Tobiška, Petr - Trávníček, Petr - Vícha, Jakub - Yushkov, Alexey … Total 373 authors
UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby galaxies.
Proceedings of Science. Vol. 395. Trieste: Sissa Medilab srl, 2022, č. článku 308. ISSN 1824-8039.
[International Cosmic Ray Conference /37./. Berlin (DE), 12.07.2021-23.07.2021]
Research Infrastructure: AUGER-CZ II - 90102
Institutional support: RVO:68378271
Keywords : surface-detector * ultra-high energy cosmic rays
OECD category: Particles and field physics
https://pos.sissa.it/395/308/pdf
The distribution of ultra-high-energy cosmic-ray arrival directions appears to be nearly isotropic except for a dipole moment of order 6×(E/10 EeV) per cent. Nonetheless, at the highest energies, as the number of possible candidate sources within the propagation horizon and the magnetic deflections both shrink, smaller-scale anisotropies might be expected to emerge. On the other hand, the flux suppression reduces the statistics available for searching for such anisotropies. In this work, we consider two different lists of candidate sources: a sample of nearby starburst galaxies and the 2MRS catalog tracing stellar mass within 250 Mpc.
Permanent Link: https://hdl.handle.net/11104/0336550
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