Detailed studies of the response of the VATLY water Cherenkovdetector, a replica of those used in the ground array of the PierreAuger Observatory, are presented with emphasis on the response to lowamplitude signals. The method used is to detect decay electrons frommuons stopping in the water volume. Results include properties of the detection process as well as of the atmospheric cosmic ray flux
The Auger Observatory water Cherenkov detectors (WCD) will require that the initial calibration and ...
The concept of a small, single-layer water Cherenkov detector, with three photomultiplier tubes (PMT...
Measurements of cosmic ray electron+positron spectrum above 10 TeV with ground-based experiments is ...
The Pierre Auger Observatory operates a hybrid detector composed of a Fluorescence Detector and a Su...
To be published in the ProceedingsInternational audienceThe ground array of the Pierre Auger Observa...
We describe a prototype water Cherenkov counter which has been built and tested with relativistic co...
Muons decaying in the water volume of a Cherenkov detector of the Pierre Auger Observatory provide a...
Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measur...
An experiment on the measurements of the energy deposit of inclined cosmic ray muon bundles is being...
A muon telescope based on 8 water cherenkov detectors was mounted at Basic Environmental Observatory...
The ground array of the Pierre Auger Observatory will consist of 1600 water-Cherenkov detectors. Suc...
An array of 1600 water Cherenkov detectors (WCDs) will form the backbone of the Pierre Auger Observa...
The Auger Observatory water Cherenkov detectors (WCD) will require that the initial calibration and ...
The concept of a small, single-layer water Cherenkov detector, with three photomultiplier tubes (PMT...
Measurements of cosmic ray electron+positron spectrum above 10 TeV with ground-based experiments is ...
The Pierre Auger Observatory operates a hybrid detector composed of a Fluorescence Detector and a Su...
To be published in the ProceedingsInternational audienceThe ground array of the Pierre Auger Observa...
We describe a prototype water Cherenkov counter which has been built and tested with relativistic co...
Muons decaying in the water volume of a Cherenkov detector of the Pierre Auger Observatory provide a...
Extensive air showers, originating from ultra-high energy cosmic rays, have been successfully measur...
An experiment on the measurements of the energy deposit of inclined cosmic ray muon bundles is being...
A muon telescope based on 8 water cherenkov detectors was mounted at Basic Environmental Observatory...
The ground array of the Pierre Auger Observatory will consist of 1600 water-Cherenkov detectors. Suc...
An array of 1600 water Cherenkov detectors (WCDs) will form the backbone of the Pierre Auger Observa...
The Auger Observatory water Cherenkov detectors (WCD) will require that the initial calibration and ...
The concept of a small, single-layer water Cherenkov detector, with three photomultiplier tubes (PMT...
Measurements of cosmic ray electron+positron spectrum above 10 TeV with ground-based experiments is ...