Using 640 days of KM3NeT/ARCA data, the collaboration finds no significant diffuse astrophysical neutrino flux and sets upper limits for all-sky and Galactic Ridge emission.
The probability density function of the arrival time of \v{C}erenkov light
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abstract
The probability density function of the arrival time of \v{C}erenkov light on a photo-multiplier tube has been studied. This study covers light production, transmission and detection. The light production includes the light from a muon, the light from a shower and the light due to the energy loss of a muon. For the transmission of light, the effects of dispersion, absorption and scattering in the medium are considered. For the detection of light, the angular acceptance and the quantum efficiency of the photo-multiplier tube are taken into account.
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Search for an all-sky and a Galactic Ridge diffuse neutrino emission with the first 2 years of KM3NeT/ARCA data
Using 640 days of KM3NeT/ARCA data, the collaboration finds no significant diffuse astrophysical neutrino flux and sets upper limits for all-sky and Galactic Ridge emission.