Status report on the ANTARES Neutrino Telescope

被引:0
作者
Vallage, Bertrand [1 ]
机构
[1] CEA Saclay, DSM Dapnia, F-91191 Gif Sur Yvette, France
来源
TAUP2007: TENTH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS | 2008年 / 120卷
关键词
D O I
10.1088/1742-6596/120/6/062008
中图分类号
O59 [应用物理学];
学科分类号
摘要
After a long and fruitful R&D phase to validate its detector concept, the ANTARES collaboration will complete by 2008 the deployment of its 12-string underwater detector at a depth of 2500 m in the Mediterranean Sea, 40 km south-east of the French town of Toulon The 3D array of 900 photomultiplier tubes (PMT) will allow high energy neutrino astronomy with a pointing accuracy better than 1 degree. The detector size grew by steps from 1 line in March 2006, to 5 lines in January 2007, sketching a real 3D detector. Data recorded continuously provide a precise calibration of the charge and arrival time of Cerenkov photons coming from muon tracks. The position and orientation of individual detectors axe measured frequently by compasses, tiltmeters and external acoustic triangulation. The data from the 3D detector allow the reconstruction of downward going cosmic ray muons and the search for the first upward going neutrino induced muons. Preliminary results of these analysis axe presented.
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