SCHÜSSLER, F.; BACKES, M.; BALZER, A.; BRUN, F.; FÜSSLING, M.; HOISCHEN, C.; LENAIN, J-P.; LORENTZ, M.; LYPOVA, I.; OHM, S.; PARSONS, D.; REIMER, A.

doi:10.1063/1.4968989

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SCHÜSSLER, F.
Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU]

BACKES, M.

BALZER, A.

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Communication dans un congrès

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AIP Conf.Proc., AIP Conf.Proc., 2016-07-11, Heidelberg. 2017, vol. 1792, n° 1, p. 060006

Resumen en inglés

The observation of an astrophysical flux of high-energy neutrinos by the IceCube collaboration opened the path to multi-messenger studies searching for the origin of high-energy cosmic rays since the detected neutrinos possibly originate in hadronic interactions near cosmic-ray accelerators. Although the neutrino sky map shows no indication of localized sources so far, the angular resolution of individual track-like events is sufficiently small to search for associated gamma-ray emission with Imaging Atmospheric Cherenkov Telescopes like H.E.S.S.Here we present the H.E.S.S. multi-messenger program to follow up on high-energy neutrino events. We show first results from searches for high-energy gamma-ray emission in spatial coincidence with neutrino events detected by the IceCube and ANTARES neutrino telescopes and discuss recent extensions towards a fully integrated real-time alert system between neutrino telescopes and the H.E.S.S. gamma-ray experiment.< Leer menos

Palabras clave en inglés

gamma ray: emission

neutrino: detector

HESS

hadronic

cosmic radiation

IceCube

angular resolution

Cherenkov counter

accelerator

imaging

ANTARES

flux

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The H.E.S.S. multi-messenger program: Searches for TeV gamma-ray emission associated with high-energy neutrinos

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