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ANTARES: the first undersea neutrino telescope

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arxiv 1104.1607 v2 pith:CILIY6UT submitted 2011-04-08 astro-ph.IM

ANTARES Collaboration This is my paper · ORCID
classification astro-ph.IM
keywords neutrinotelescopeantaresdetectorfirstapparatusastronomycompleted
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The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational Neutrino Telescope in the Mediterranean Sea. The main purpose of the detector is to perform neutrino astronomy and the apparatus also offers facilities for marine and Earth sciences. This paper describes the design, the construction and the installation of the telescope in the deep sea, offshore from Toulon in France. An illustration of the detector performance is given.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Detecting and Studying High-Energy Collider Neutrinos with FASER at the LHC

    hep-ex 2019-08 accept novelty 7.0 of 10

    FASERν is predicted to detect thousands of collider neutrinos at the LHC and measure their cross sections at TeV energies, closing a gap in neutrino measurements.

  2. Search for Magnetic Monopoles with the Complete ANTARES Dataset

    hep-ex 2025-05 conditional novelty 5.0 of 10

    After 14 years of ANTARES data, no magnetic monopole candidates were found, yielding 90% confidence flux upper limits down to about 6e-19 cm^-2 s^-1 sr^-1.

  3. Atmospheric Cherenkov Telescopes as a Potential Veto Array for Neutrino Astronomy

    astro-ph.IM 2019-08 conditional novelty 5.0 of 10

    A roughly 250-telescope IACT veto array could reject atmospheric neutrinos above 15-30 TeV and increase IceCube event rates from overhead sources by factors of 3 to 13.

  4. Fermion Dark Matter and Radiative Neutrino Masses from Spontaneous Lepton Number Breaking

    hep-ph 2019-08 conditional novelty 4.0 of 10

    In the scotogenic model with spontaneous lepton number breaking, the lightest heavy Majorana neutrino can be a sub-TeV dark matter particle with the correct relic abundance in three mass windows, while evading current...

  5. Active Galactic Nuclei as high-energy neutrino sources

    astro-ph.HE 2026-06 unverdicted novelty 2.5 of 10

    Review summarizing correlations between astrophysical neutrinos and gamma-ray/radio AGN, specific source associations, proposed production mechanisms, and future prospects.

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