Understand
The ANTARES telescope is being built in the Mediterranean Sea.
- The detector consists of a 3D array of photomultipliers (PMTs) that detects the Cherenkov light induced by the muons produced in neutrino interactions.
- Other signatures can also be detected.
- Since the neutrino fluxes from point-like sources are expected to be small, it is of the utmost importance to take advantage of the ANTARES pointing accuracy (angular resolution better than 0.3 degrees for muon events above 10 TeV) to disentangle a possible signal from the unavoidable atmospheric neutrino background.
Built on
Maximum likelihood from incomplete data via the em algorithm
A. P. Dempster et al · 1977
Earlier work this paper cites.
A deep sea telescope of high energy neutrinos
ANTARES Collaboration · 1999
Earlier work this paper cites.
Neutrino astronomy with the MACRO detector
M. Ambrosio et al · 2001
Earlier work this paper cites.
Similar
PhD thesis, Universitat de València, Spain, 2003
E. Carmona · 2003
Cited alongside, same era.
PhD thesis, Universiteit van Amsterdan, 2004
A. Heijboer · 2004
Cited alongside, same era.
Then
Search for extraterrestrial point sources of neutrinos with AMANDA-II
J. Ahrens et al · 2004
Later among the works it cites.
Sensitivity of IceCube detector to astrphysical sources of high energy muon neutrinos
J. Ahrens et al · 2004
Later among the works it cites.
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