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On the potential of Cherenkov Telescope Arrays and KM3 Neutrino Telescopes for the detection of extended sources

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00546822" target="_blank" >RIV/68378271:_____/18:00546822 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1016/j.astropartphys.2018.03.001" target="_blank" >https://doi.org/10.1016/j.astropartphys.2018.03.001</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.astropartphys.2018.03.001" target="_blank" >10.1016/j.astropartphys.2018.03.001</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    On the potential of Cherenkov Telescope Arrays and KM3 Neutrino Telescopes for the detection of extended sources

  • Original language description

    We discuss the discovery potential of extended Very-High-Energy (VHE) neutrino sources by the future KM3 Neutrino Telescope (KM3NeT) in the context of the constraining power of the Cherenkov Telescope Array (CTA), designed for deep surveys of the sky in VHE gamma rays. The study is based on a comparative analysis of sensitivities of KM3NeT and CTA. We show that a minimum gamma-ray energy flux of E-2 Phi(gamma) (10 TeV) > 1 x 10(-12) TeV cm(-2) s (-1) is required to identify a possible neutrino counterpart with a 3 sigma significance and 10 years of KM3NeT observations with upgoing muons, if the source has an angular size of R-STC = 0.1 degrees and emits gamma rays with an E-2 energy spectrum through a full hadronic mechanism. This minimum gamma-ray flux is increased to the level of E-2 phi(gamma) (10 TeV) > 2 x 10(-11) TeV cm(-2) s(-1) in case of sources with radial extension of R-STC = 2.0 degrees.n

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

  • Continuities

Others

  • Publication year

    2018

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astroparticle Physics

  • ISSN

    0927-6505

  • e-ISSN

    1873-2852

  • Volume of the periodical

    100

  • Issue of the periodical within the volume

    July

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    11

  • Pages from-to

    69-79

  • UT code for WoS article

    000430624000008

  • EID of the result in the Scopus database

    2-s2.0-85044102528