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The Antares And Km3Net Neutrino Telescopes: Status And Outlook For Acoustic Studies

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Figure

Figure 1. Left: The ANTARES detector configuration, showing the 12 lines hosting standard storeys withoptical modules (in black), as well as the instrumented line (IL07)
Figure 1. Left: The ANTARES detector configuration, showing the 12 lines hosting standard storeys withoptical modules (in black), as well as the instrumented line (IL07)
Figure 3. Left: Rate of multiple coincidences in a 25 ns time window for the lowermost DOM (DOM1) ofARCA-DU1 and for the uppermost DOM (DOM18) of ARCA-DU2, as compared to Monte Carlo predictions.Right: Distribution of reconstructed zenith angle θ for ORC -DU1 data, atmospheric neutrino and atmosphericmuon Monte Carlos.

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