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The ANTARES project
T. Montaruli
The ANTARES deep-sea neutrino telescope will be located at a depth of 2400 m in the Mediterranean Sea. Deployment of the detector will commence this Autumn and is expected to be co…
Measurement of the residual energy of muons in the Gran Sasso underground Laboratories
The MACRO Collaboration, M. Ambrosio
The MACRO detector was located in the Hall B of the Gran Sasso underground Laboratories under an average rock overburden of 3700 hg/cm^2. A transition radiation detector composed o…
Status Report of the MACRO Experiment for the year 2001
G. Giacomelli, A. Margiotta
In this 2001 status report of the MACRO experiment, results are presented on atmospheric neutrinos and neutrino oscillations, high energy neutrino astronomy, searches for WIMPs, se…
The FLUKA atmospheric neutrino flux calculation
G. Battistoni, A. Ferrari, T. Montaruli +1
The 3-dimensional (3-D) calculation of the atmospheric neutrino flux by means of the FLUKA Monte Carlo model is here described in all details, starting from the latest data on prim…
Sedimentation and Fouling of Optical Surfaces at the ANTARES Site
ANTARES collaboration
ANTARES is a project leading towards the construction and deployment of a neutrino telescope in the deep Mediterranean Sea. The telescope will use an array of photomultiplier tubes…
Search for cosmic ray sources using muons detected by the MACRO experiment
M. Ambrosio
The MACRO underground detector at Gran Sasso Laboratory recorded 60 million secondary cosmic ray muons from February 1989 until December 2000. Different techniques were used to ana…