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Search for a cosmic point-like neutrino source from the direction of the ultra-high-energy event KM3-230213A

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F25%3A00389193" target="_blank" >RIV/68407700:21670/25:00389193 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.22323/1.501.1110" target="_blank" >https://doi.org/10.22323/1.501.1110</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.501.1110" target="_blank" >10.22323/1.501.1110</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Search for a cosmic point-like neutrino source from the direction of the ultra-high-energy event KM3-230213A

  • Original language description

    On February 13, 2023, the KM3NeT/ARCA neutrino telescope detected an ultra-high-energy neutrino event, KM3-230213A, with an estimated energy of approximately 220 PeV - the most energetic neutrino ever observed. This unprecedented event marks a significant milestone in the field of astroparticle physics, offering new insights into the potential sources of these extreme astrophysical phenomena. In this work, we present a follow-up analysis aimed at identifying a potential cosmic point-like neutrino source associated with KM3-230213A. We perform a dedicated search for a cluster of neutrino events in the direction of KM3-230213A using data from KM3NeT/ARCA, KM3NeT/ORCA, ANTARES and IceCube. In order to assess the potential spatial clustering of neutrino events around KM3-230213A, we employ either an ON/OFF technique or a maximum-likelihood method. This contribution presents the methodology, the datasets used, the event selection criteria, and the statistical methods applied. We discuss the results in the context of multi-messenger astrophysics, highlighting their implications for the origin of the ultra-high-energy neutrino KM3-230213A.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/LM2023063" target="_blank" >LM2023063: Laboratoire Souterrain de Modane – participation of the Czech Republic</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

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

    39th International Cosmic Ray Conference (ICRC2025)

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

  • Number of pages

    13

  • Pages from-to

    1-13

  • Publisher name

    PoS - Proceedings of Science, Sissa Medialab srl

  • Place of publication

    Trieste

  • Event location

    Geneva

  • Event date

    Jul 14, 2025

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article