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The latest result on UHE-photons 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%3A00640472" target="_blank" >RIV/68378271:_____/25:00640472 - isvavai.cz</a>

  • Alternative codes found

    RIV/61989592:15310/25:73634831

  • Result on the web

    <a href="https://www.epj-conferences.org/articles/epjconf/pdf/2025/04/epjconf_ricap2024_06008.pdf" target="_blank" >https://www.epj-conferences.org/articles/epjconf/pdf/2025/04/epjconf_ricap2024_06008.pdf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/epjconf/202531906008" target="_blank" >10.1051/epjconf/202531906008</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The latest result on UHE-photons at the Pierre Auger Observatory

  • Original language description

    The Pierre Auger Observatory is the most sensitive detector to primary photons with energies above 0.2 EeV providing unprecedented exposure to ultrahigh- energy (UHE) cosmic rays and specifically to UHE photons. The Observatory measures extensive air showers using a hybrid technique that combines a fluorescence detector (FD) with a ground array of particle detectors (SD). The signatures of a photon-induced air shower are a larger atmospheric depth of the shower maximum (Xmax) and a steeper lateral distribution function, along with a lower number of muons with respect to the bulk of hadron-induced background. Using observables measured by the FD and SD, various photon searches in different energy bands are performed. These efforts have produced some of the most stringent upper limits on the diffuse fluxes of UHE photons. These limits place significant constraints on current models for the origin of UHE cosmic rays, highlighting the leading role of the Observatory in multimessenger astronomy at the highest energies. In this contribution, an overview of current activities related to the search for UHE photons is shown, using more than 15 years of data from the Pierre Auger Observatory. The latest results of the searches for diffuse fluxes of photons will be presented, as well as follow-up searches for UHE photons in association with transient events, such as gravitational wave events, will be summarized.

  • 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

    EPJ Web of Conferences

  • ISBN

  • ISSN

    2100-014X

  • e-ISSN

  • Number of pages

    4

  • Pages from-to

    06008

  • Publisher name

    E D P Science

  • Place of publication

    Les Ulis

  • Event location

    Roma

  • Event date

    Sep 23, 2024

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    001448416000027