Mar 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1213..249v&link_type=abstract
FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP Conference Proceedings, Volume 1213, pp. 249-251 (2010).
Other
Astronomical Telescopes, Gamma-Rays, Monte Carlo Methods, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors, Gamma-Ray, Monte Carlo Simulations
Scientific paper
The R&D activities of the NEMO Collaboration for the construction of a km3 scale underwater neutrino telescope are described. Results from about 10 years of site seeking and monitoring activities have demonstrated that a wide abyssal plain, about 80 km off-shore Capo Passero (Sicily), is the optimal site for the installation of the telescope. With the pilot project NEMO Phase-1, the NEMO Collaboration realized and installed at 2000 m depth at the underwater Test Site of the Laboratori Nazionali del Sud a fully equipped deep-sea facility to test prototypes and develop new technologies for a km3 neutrino telescope. The realization of an underwater infrastructure at 3500 m on the Capo Passero site is in progress (NEMO Phase-2). It will enable the validation of the technological solutions proposed at depths needed for the final km3 detector and a long term monitoring of the selected site.
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