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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

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • 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

  • ISSN

    1824-8039

  • e-ISSN

  • 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