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Extragalactic Blazar Diffuse Population Interpretation for the KM3-230213A event

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F25%3A00389245" target="_blank" >RIV/68407700:21670/25:00389245 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.22323/1.501.0986" target="_blank" >https://doi.org/10.22323/1.501.0986</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.501.0986" target="_blank" >10.22323/1.501.0986</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Extragalactic Blazar Diffuse Population Interpretation for the KM3-230213A event

  • 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 in the hundreds of PeV range. In this study, we explore whether such a rare event can originate from a diffuse population of blazars. We simulate the neutrino and photon emission from blazar jets using the AM3 lepto-hadronic code, convolve the results with the Fermi-LAT blazar luminosity function, and evaluate the resulting diffuse flux. A likelihood analysis incorporating both KM3NeT and IceCube exposure data, as well as a gamma-ray background penalty from Fermi-LAT, allows us to constrain the parameter space of the baryonic loading and proton spectral index. We find that the KM3-230213A event could have been generated by a blazar diffuse flux, under physically motivated assumptions. This work demonstrates the strength of multi-messenger analyses and underlines the importance of joint neutrino observatory efforts in interpreting the high-energy sky.

  • 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

    10

  • Pages from-to

    1-10

  • 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