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Time Calibration of the ANTARES Neutrino Telescope

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Academic year: 2021

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Figure

Fig. 1. Schematic view of the ANTARES detector, consisting of twelve mooring lines connected to the shore station through an electro-optical cable
Fig. 3. Time offset due to the walk effect as a function of the PMT pulse amplitude in units of photo-electrons.
Fig. 4. Schematic view of the clock system: optical signals are sent from shore and propagated up to the junction box where they are split towards the SCMs of the different lines
Fig. 6. Left: Time evolution of the difference in the round-trip times between the shore and an SCM and one of the LCMs
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