Amplifying UHECR arrival direction information using mass estimators at the Pierre Auger Observatory
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F25%3A00640403" target="_blank" >RIV/68378271:_____/25:00640403 - isvavai.cz</a>
Alternative codes found
RIV/61989592:15310/25:73635009
Result on the web
<a href="https://pos.sissa.it/484/068/pdf" target="_blank" >https://pos.sissa.it/484/068/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.484.0068" target="_blank" >10.22323/1.484.0068</a>
Alternative languages
Result language
angličtina
Original language name
Amplifying UHECR arrival direction information using mass estimators at the Pierre Auger Observatory
Original language description
The origin of Ultra-High-Energy Cosmic Rays (UHECRs) is one of the biggest mysteries in modern astrophysics. Since UHECRs are deflected by Galactic and extragalactic magnetic fields, their arrival directions do not point to their sources. Previous analyses conducted on the arrival directions of high-energy events (E≥32EeV ) recorded by the Surface Detector of the Pierre Auger Observatory have not shown significant anisotropies. The largest excess found in the first 19 years of data - at the 4.0σ level - is in the region around Centaurus A, and it is also the driving force of a correlation of UHECR arrival directions with a catalog of Starburst Galaxies, which is at the 3.8σ level. Since UHECRs are mostly nuclei, the lightest ones (least charged) are also the least deflected. While the mass of the events can be estimated better using the Fluorescence Detector of the Pierre Auger Observatory, the Surface Detector provides the necessary statistics needed for astrophysical studies. The introduction of novel mass-estimation techniques, such as machine learning models and an algorithm based on air-shower universality, will help identify high-rigidity events in the Surface Detector data of the Pierre Auger Observatory. With this work, we present how event-per-event mass estimators can help enhance the sensitivity in the search for anisotropies in the arrival directions of UHECRs at small and intermediate angular scales using simulations.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10303 - Particles and field physics
Result continuities
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
Others
Publication year
2025
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of Science
ISBN
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ISSN
1824-8039
e-ISSN
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Number of pages
8
Pages from-to
068
Publisher name
Sissa Medilab srl
Place of publication
Trieste
Event location
Malargüe
Event date
Nov 17, 2024
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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