Published 2009
| Version v1
Journal article
The Antares neutrino detectors
Description
The Antares neutrino telescope, operating at 2.5 km depth in the Mediterranean Sea, 40 km off the Toulon shore, represents the worlds largest operational underwater neutrino telescope, optimised for the detection of Cherenkov light produced by neutrino-induced muons. The neutrinos momentum is transferred to the muons allowing for reconstruction of the direction of the neutrino. The main goal of Antares is the search of high-energy neutrinos from astrophysical point or transient sources. Antares has been taking data in its full 12 lines configuration since May 2008: in these Proceedings the description of the detector and its performances will be presented while first preliminary results on neutrino events will be discussed.
Additional details
Publishing Information
- Journal Title
- Nuovo Cimento della Societa Italiana di Fisica. C, Geophysics and Space Physics
- Journal Volume
- 32
- Journal Issue
- 3-4
- Journal Page Range
- p. 347-351
- ISSN
- 1124-1896
Conference
- Title
- Incontri di Fisica delle Alte Energie 2009
- Acronym
- IFAE 2009
- Dates
- 15-17 Apr 2009
- Place
- Bari (Italy)
INIS
- Country of Publication
- Italy
- Country of Input or Organization
- Italy
- INIS RN
- 42017590
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CHERENKOV COUNTERS; COSMIC NEUTRINOS; COSMIC RADIATION; COSMIC RAY DETECTION; WEAK INTERACTIONS
- Descriptors DEC
- BASIC INTERACTIONS; COSMIC RADIATION; DETECTION; ELEMENTARY PARTICLES; FERMIONS; INTERACTIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MEASURING INSTRUMENTS; NEUTRINOS; RADIATION DETECTION; RADIATION DETECTORS; RADIATIONS