Neutrino Astronomy with ANTARES

Details Neutrino Astronomy with ANTARES Neutrino Astronomy with ANTARES

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..491e&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

The ANTARES collaboration is building a high energy neutrino telescope in the Mediterranean sea, at a depth of 2500 m, 40 km off the French coast. This instrument will detect Cherenkov light produced in sea water by neutrino-induced muons. ANTARES will provide an alternative to the photon and cosmic ray observations in astrophysics. Preliminary results of a small size prototype, currently operating, will be presented. The first line of ANTARES will be deployed this autumn and the detector should be fully operational by mid-2007.

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