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Sensitivity of an underwater Cerenkov km3 telescope to TeV neutrinos from Galactic Microquasars
C. Distefano, the NEMO Collaboration
In this paper are presented the results of Monte Carlo simulations on the capability of the proposed NEMO-km telescope to detect TeV muon neutrinos from Galactic microquasars.…
The primary cosmic ray composition between 10**15 and 10**16 eV from Extensive Air Showers electromagnetic and TeV muon data
TOP Collaboration, MACRO Collaboration
The cosmic ray primary composition in the energy range between 10**15 and 10**16 eV, i.e., around the "knee" of the primary spectrum, has been studied through the combined measurem…
The Search for the Sidereal and Solar Diurnal Modulations in the Total MACRO Muon Data Set
The MACRO Collaboration, M. Ambrosio
We have analyzed 44.3M single muons collected by MACRO from 1991 through 2000 in 2,145 live days of operation. We have searched for the solar diurnal, apparent sidereal, and pseudo…
Search for diffuse neutrino flux from astrophysical sources with MACRO
The MACRO Collaboration
Many galactic and extragalactic astrophysical sources are currently considered promising candidates as high energy neutrino emitters. Astrophysical neutrinos can be detected as upw…
The ANTARES Optical Module
The ANTARES Collaboration
The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equi…