To measure cosmic rays at the highest energies, ground based detectors sparsely covering an area of several thousand square kilometers to detect cosmic ray induced air showers are used. One of those experiments is the Pierre Auger Observatory, which is currently being upgraded for a better determination of the muonic component in the showers to allow a better identification of the type of primary particle. For this upgrade multiple different detector concepts and designs were proposed. One of those proposals is the Aachen Muon Detector (AMD), which is a tiled scintillator detector with silicon photomultipliers (SiPMs) as light sensors. To digitize the SiPM signals the EASIROC chip is used, which allows to read out 32 SiPMs and adjusting of ...
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to...
© 2017 IOP Publishing Ltd and Sissa Medialab srl. AMIGA (Auger Muons and Infill for the Ground Array...
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory de...
To measure cosmic rays at the highest energies, ground based detectors sparsely covering an area of ...
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to...
© 2017 IOP Publishing Ltd and Sissa Medialab srl. AMIGA (Auger Muons and Infill for the Ground Array...
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory de...
To measure cosmic rays at the highest energies, ground based detectors sparsely covering an area of ...
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to...
© 2017 IOP Publishing Ltd and Sissa Medialab srl. AMIGA (Auger Muons and Infill for the Ground Array...
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory de...