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AMIGA at the Auger observatory: the telecommunications system
(Iop Publishing, 2013-12)
AMIGA is an extension of the Pierre Auger Observatory that will consist of 85 detector pairs, each one composed of a surface water-Cherenkov detector and a buried muon counter. Each muon counter has an area of 30 square ...
Digital electronics for the Pierre Auger Observatory AMIGA muon counters
(Iop Publishing, 2014-04)
The ``Auger Muons and Infill for the Ground Array´´ (AMIGA) project provides direct muon counting capacity to the Pierre Auger Observatory and extends its energy detection range down to 0.3 EeV. It currently consists of ...
The Amiga Enhancement Of The Pierre Auger Observatory
(IOP PUBLISHING LTDBRISTOL, 2015)
Sistema de adquisición de datos para la extensión “Amiga” del observatorio Pierre Auger
(Universidad Michoacana de San Nicolás de Hidalgo, 2008-02)
The present thesis focuses around the design and implementation of the system of acquisition of data from a prototype muon detector called BATATA [x] (Buried Array Telescope at Auger) that will be installed as part of the ...
Design and implementation of the AMIGA embedded system for data acquisition
(IOP Publishing, 2022)
AMIGA at the Pierre Auger Observatory: The interface and control electronics of the first prototype muon counters
(Elsevier Science, 2015-04)
AMIGA is an enhancement of the Pierre Auger Observatory. The main goals of AMIGA are to extend the full efficiency range to low erenergies of the Observatory and to measure the muon content of extensive air showers. ...
Search for ultra-high energy photons with the AMIGA muon detector
(2018-02-09)
Los rayos cósmicos (E > 1014 eV) son conocidos desde hace más de 70 años y, sin embargo, su origen sigue siendo un misterio. Del mismo modo, la posibilidad de una componente fotónica de muy alta energía en el flujo de ...
Optoelectrónica con Fotomultiplicadores de Silicio para Detectores de Rayos Cósmicos.
(Escuela de Posgrado - Facultad Regional Buenos Aires, 2018)