The ground array of the Pierre Auger Observatory will consist of 1600 water-Cherenkov detectors. Such detectors give signals which can help differentiate between muons and electrons in extensive air showers. The relative numbers of muons and electrons is sensitive to the type of primary particle which initiated the shower. Results are presented using methods which describe the muon content and related information, such as the time structure of the shower front
We present a new method for probing the hadronic interaction models at ultrahigh energy and extracti...
The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The si...
The mass composition of ultra-high energy cosmic rays is a critical issue to understand their origin...
The ground array of the Pierre Auger Observatory will consist of 1600 water-Cherenkov detectors. Suc...
To be published in the ProceedingsInternational audienceThe ground array of the Pierre Auger Observa...
An array of 1600 water Cherenkov detectors (WCDs) will form the backbone of the Pierre Auger Observa...
We report the results of a study of the response of a Pierre Auger water tank to electrons of a few ...
Muons decaying in the water volume of a Cherenkov detector of the Pierre Auger Observatory provide a...
The muon content of extensive air showers is an observable sensitive to the primary composition and ...
Abstract: Applying different filtering techniques to the temporal distribution of the signals measur...
Several methods for estimating the muonic part of the signal observed in the surface Cherenkov detec...
Abstract. We consider a ground array of scintillation and water Cherenkov detectors with the purpose...
We present a new method for probing the hadronic interaction models at ultrahigh energy and extracti...
The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The si...
The mass composition of ultra-high energy cosmic rays is a critical issue to understand their origin...
The ground array of the Pierre Auger Observatory will consist of 1600 water-Cherenkov detectors. Suc...
To be published in the ProceedingsInternational audienceThe ground array of the Pierre Auger Observa...
An array of 1600 water Cherenkov detectors (WCDs) will form the backbone of the Pierre Auger Observa...
We report the results of a study of the response of a Pierre Auger water tank to electrons of a few ...
Muons decaying in the water volume of a Cherenkov detector of the Pierre Auger Observatory provide a...
The muon content of extensive air showers is an observable sensitive to the primary composition and ...
Abstract: Applying different filtering techniques to the temporal distribution of the signals measur...
Several methods for estimating the muonic part of the signal observed in the surface Cherenkov detec...
Abstract. We consider a ground array of scintillation and water Cherenkov detectors with the purpose...
We present a new method for probing the hadronic interaction models at ultrahigh energy and extracti...
The detectors of the surface array of the Pierre Auger Observatory are water Cherenkov tanks. The si...
The mass composition of ultra-high energy cosmic rays is a critical issue to understand their origin...