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Measuring the atmospheric neutrino oscillation parameters and constraining the 3+1 neutrino model with ten years of ANTARES data
ANTARES Collaboration, A. Albert, M. André +133
The ANTARES neutrino telescope has an energy threshold of a few tens of GeV. This allows to study the phenomenon of atmospheric muon neutrino disappearance due to neutrino oscillat…
Search for Multi-messenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during its first Observing Run, ANTARES and IceCube
ANTARES, IceCube, LIGO +1589
Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-th…
Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources
The KM3NeT Collaboration, S. Aiello, S. E. Akrame +219
KM3NeT will be a network of deep-sea neutrino telescopes in the Mediterranean Sea. The KM3NeT/ARCA detector, to be installed at the Capo Passero site (Italy), is optimised for the…
The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope
A. Albert, M. André, M. Anghinolfi +124
One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are importa…
Search for neutrinos from TXS 0506+056 with the ANTARES telescope
A. Albert, M. Andrè, M. Anghinolfi +124
The results of three different searches for neutrino candidates, associated with the IceCube-170922A event or from the direction of TXS 0506+056, by the ANTARES neutrino telescope…
Long-term monitoring of the ANTARES optical module efficiencies using decays in sea water
ANTARES collaboration, A. Albert, M. André +124
Cherenkov light induced by radioactive decay products is one of the major sources of background light for deep-sea neutrino telescopes such as ANTARES. These decays are at the same…