Muons decaying in the water volume of a Cherenkov detector of the Pierre Auger Observatory provide a useful calibration point at low energy. Using the digitized waveform continuously recorded by the electronics of each tank, we have devised a simple method to extract the charge spectrum of the Michel electrons, whose typical signal is about 1/8 of a crossing vertical muon. This procedure, moreover, allows continuous monitoring of the detector operation and of its water level. We have checked the procedure with high statistics on a test tank at the Observatory base and applied with success on the whole array
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies (\u3e 1019 eV...
To obtain direct measurements of the muon content of extensive air showers with energy above 101 eV,...
Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measur...
Muons decaying in the water volume of a Cherenkov detector of the Pierre Auger Observatory provide a...
The Auger Observatory water Cherenkov detectors (WCD) will require that the initial calibration and ...
The ground array of the Pierre Auger Observatory will consist of 1600 water-Cherenkov detectors. Suc...
Detailed studies of the response of the VATLY water Cherenkovdetector, a replica of those used in th...
The muon content of extensive air showers is an observable sensitive to the primary composition and ...
To be published in the ProceedingsInternational audienceThe ground array of the Pierre Auger Observa...
The Pierre Auger Observatory operates a hybrid detector composed of a Fluorescence Detector and a S...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
An experiment on the measurements of the energy deposit of inclined cosmic ray muon bundles is being...
In this work we used a particle detector and a digital oscilloscope to measure the mean life time of...
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies (\u3e 1019 eV...
To obtain direct measurements of the muon content of extensive air showers with energy above 101 eV,...
Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measur...
Muons decaying in the water volume of a Cherenkov detector of the Pierre Auger Observatory provide a...
The Auger Observatory water Cherenkov detectors (WCD) will require that the initial calibration and ...
The ground array of the Pierre Auger Observatory will consist of 1600 water-Cherenkov detectors. Suc...
Detailed studies of the response of the VATLY water Cherenkovdetector, a replica of those used in th...
The muon content of extensive air showers is an observable sensitive to the primary composition and ...
To be published in the ProceedingsInternational audienceThe ground array of the Pierre Auger Observa...
The Pierre Auger Observatory operates a hybrid detector composed of a Fluorescence Detector and a S...
International audienceIn this work, a water tank muon spectrometer was designed, assembled and opera...
An experiment on the measurements of the energy deposit of inclined cosmic ray muon bundles is being...
In this work we used a particle detector and a digital oscilloscope to measure the mean life time of...
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies (\u3e 1019 eV...
To obtain direct measurements of the muon content of extensive air showers with energy above 101 eV,...
Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measur...