Muon counting using silicon photomultipliers in the AMIGA detector of the Pierre Auger observatory

AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory designed to extend its energy range of detection and to directly measure the muon content of the cosmic ray primary particle showers. The array will be formed by an infill of surface water-Cherenkov det...

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Guardado en:
Detalles Bibliográficos
Autor principal: Multitudinario:424
Formato: JOUR
Materias:
Front-end electronics for detector readout
Pattern recognition, cluster finding, calibration and fitting methods
Performance of high energy physics detectors
Photon detectors for UV, visible and IR photons (solid-state) (PIN diodes, APDs, Si-PMTs, G-APDs, CCDs, EBCCDs, EMCCDs etc)
Augers
Charged particles
Cosmic rays
Cosmology
High energy physics
Observatories
Pattern recognition
Photomultipliers
Photons
Scintillation
Semiconductor diodes
Surface waters
Detector readout
Fitting method
Front end electronics
High energy physics detector
Pierre Auger observatory
PiN diode
Silicon photomultiplier
Water Cherenkov detectors
Silicon detectors
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17480221_v12_n3_p_Multitudinario
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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