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An algorithm for the reconstruction of neutrino-induced showers in the ANTARES neutrino telescope

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Academic year: 2021

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Figure 1: Geometric variables considered by the likelihood function in equation (8): pho-ton emission angle φ i , shower–
Figure 2: Unbiased distribu- distribu-tion of the charge caused by environmental and atmospheric background.
Figure 3: Distance between the true position of the neutrino inter- inter-action vertex and the reconstructed shower position in the longitudinal (left) and perpendicular (right) directions along the neutrino axis
Figure 4: Left: Median angle between the directions of the reconstructed shower and the Monte Carlo neutrino as a function of the neutrino energy.
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