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Extreme blazars: stacking analysis with KM3NeT/ARCA

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F25%3A00389240" target="_blank" >RIV/68407700:21670/25:00389240 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.22323/1.501.1125" target="_blank" >https://doi.org/10.22323/1.501.1125</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.501.1125" target="_blank" >10.22323/1.501.1125</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Extreme blazars: stacking analysis with KM3NeT/ARCA

  • Original language description

    KM3NeT/ARCA is a large-scale underwater Cherenkov neutrino detector, currently under construction at the bottom of the Mediterranean Sea. The detector’s geometry is optimised for the observation of TeV-PeV astrophysical neutrinos. Once completed, the detector will consist of 230 Detection Units (DUs). Each Detection Unit is an 800-meter vertical line that holds 18 Digital Optical Modules (DOMs), each containing 31 photomultiplier tubes. In this contribution we describe the analysis on Extreme High-frequency-peaked BL Lacs (EHBLs) blazars by integrating the theoretical modeling of these blazars, performed with the LeHaMoc numerical code, and in parallel the expectations of neutrinos emitted from these sources in binned likelihood stacking analyses based on KM3NeT/ARCA’s data. We present a detailed analysis of a carefully selected sample of extreme blazars, focusing on their multiwavelength characteristics and high-energy emission mechanisms. This study represents a novel approach in the field, combining detailed modeling of the spectral energy distributions (SEDs) with a stacking sensitivity analysis tailored to this rare class of sources.

  • 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

    11

  • Pages from-to

    1-11

  • 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

    —