ANTARES: the first undersea neutrino telescope

By M. Ageron, J. Aguilar, I. A. Samarai, A. Albert, F. Ameli, M. André, M. Anghinol, G. Anton, S. Anvar, M. Ardid and 271 more. 2011

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OBSERVATION AND CHARACTERIZATION OF A COSMIC MUON NEUTRINO FLUX FROM THE NORTHERN HEMISPHERE USING SIX YEARS OF ICECUBE DATA (2016, background): “The construction of large Cherenkov detectors by instrumenting optically transparent natural media, i.e., deep oceans, lakes, and glaciers with photo-sensors (Belolaptikov et al. 1997; Andres et al. 2000; Ageron et al. 2011) proved to be a key concept.”
The SUrvey for Pulsars and Extragalactic Radio Bursts – II. New FRB discoveries and their follow-up. (2017, background): “The ANTARES telescope (Ageron et al. 2011) is a deep-sea Cherenkov neutrino detector, located 40 km off Toulon, France, in the Mediterranean Sea and dedicated to the observation of neutrinos with Eν 100 GeV.”
Multi-messenger observations of a binary neutron star merger (2017, methodology): “Neutrinos The detection of GW170817 was rapidly followed up by the IceCube (Aartsen et al. 2017) and ANTARES (Ageron et al. 2011) neutrino observatories and the Pierre Auger Observatory (Aab et al. 2015a) to search for coincident, high-energy (GeV– EeV) neutrinos emitted in the relativistic outflow…”
Detecting and studying high-energy collider neutrinos with FASER at the LHC (2019, methodology): “The measurement of forward neutrino production will be a key input for high-energy neutrino measurements by large-scale Cherenkov observatories, such as IceCube [136], ANTARES [137], Baikal-GVD [138], and KM3NeT/ARCA [139].”