Performance of the front-end electronics of the ANTARES neutrino telescope
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Performance of the front-end electronics of the ANTARES neutrino telescope

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Performance of the front-end electronics of the ANTARES neutrino telescope

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ANTARES Collaboration; Aguilar Sánchez, Juan Antonio; Bigongiari, C.; Dornic, Damien; Emanuele, U.; Gómez González, Juan Pablo; Hernández Rey, Juan José Perfil; Mangano, Salvatore; Salesa Greus, Francisco; Toscano, S.; Yepes Ramírez, Harold; Zornoza Gómez, Juan de Dios Perfil; Zúñiga Román, Juan
Aquest document és un/a article, creat/da en: 2010
ANTARES is a high-energy neutrino telescope installed in the Mediterranean Sea at a depth of 2475 m. It consists of a three-dimensional array of optical modules, each containing a large photomultiplier tube. A total of 2700 front-end ASICs named Analogue Ring Samplers (ARS) process the phototube signals, measure their arrival time, amplitude and shape as well as perform monitoring and calibration tasks. The ARS chip processes the analogue signals from the optical modules and converts information into digital data. All the information is transmitted to shore through further multiplexing electronics and an optical link. This paper describes the performance of the ARS chip; results from the functionality and characterization tests in the laboratory are summarized and the long-term performance in the apparatus is illustrated.

    ANTARES Collaboration Aguilar Sánchez, Juan Antonio Bigongiari, C. Dornic, Damien Emanuele, U. Gómez González, Juan Pablo Hernández Rey, Juan José Mangano, Salvatore Salesa Greus, Francisco Toscano, S. Yepes Ramírez, Harold Zornoza Gómez, Juan de Dios Zúñiga Román, Juan 2010 Performance of the front-end electronics of the ANTARES neutrino telescope Nuclear Instruments & Methods in Physics Research Section A-Accelerators Spectrometers Detectors and Associated Equipment 622 1 59 73
http://dx.doi.org/10.1016/j.nima.2010.06.225
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