Search for correlations between high-energy gamma rays and neutrinos with the HAWC and ANTARES detectors

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    • uploaded July 4, 2021

    Discussion timeslot (ZOOM-Meeting): 21. July 2021 - 12:00
    ZOOM-Meeting URL: https://desy.zoom.us/j/91896950007
    ZOOM-Meeting ID: 91896950007
    ZOOM-Meeting Passcode: ICRC2021
    Corresponding Session: https://icrc2021-venue.desy.de/channel/24-Ground-based-measurements-of-low-energy-GCRs-SH/98
    Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-06/7

    Abstract:
    'ANTARES is an underwater neutrino detector in the Mediterranean Sea. Its location, reconstruction accuracy for all-flavor neutrino interactions, and low energy threshold, make it the most sensitive neutrino observatory for searches below 100 TeV over large parts of the sky. The HAWC experiment is a water Cherenkov gamma-ray detector located in Mexico. Thanks to its large field of view it is an excellent instrument to observe the very-high energy gamma-ray sky and perform high-sensitivity surveys of the Galactic Plane.rnThe 10-year ANTARES data set and 3-year HAWC point source surveys are used to search for all- flavor neutrino emission in correlation with the highly-significant observations by HAWC in the gamma-ray sky by means of a maximum-likelihood template search. No significant observation for a correlation has been identified and upper limits on the neutrino flux from the HAWC observations have been set.'

    Authors: Giovanna Ferrara | for the ANTARES Collaboration | for the HAWC Collaboration
    Co-Authors: Luigi Antonio Fusco
    Collaboration: AntaresHAWC

    Indico-ID: 967
    Proceeding URL: https://pos.sissa.it/395/962

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    Presenter:

    Giovanna Ferrara


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