UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby galaxies

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00564975" target="_blank" >RIV/68378271:_____/22:00564975 - isvavai.cz</a>
Alternative codes found
RIV/61989592:15310/22:73616907
Result on the web
<a href="https://pos.sissa.it/395/308/pdf" target="_blank" >https://pos.sissa.it/395/308/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.395.0308" target="_blank" >10.22323/1.395.0308</a>

Result language
angličtina
Original language name
UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby galaxies
Original language description
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.
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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