A proposal for a new system to capture signals in the Optical Module (OM) of an underwater neutrino telescope is described. It concentrates on the problem of power consumption and time precision. In particular, a solution for the interface between the photomultiplier (PMT) and the front-end electronics is presented.
D. LO PRESTI, N. RANDAZZO, L. CAPONETTO, F. GIORGI, GABRIELLI A. (2008). Low Power Front End for the Optical Module of a Neutrino Underwater Telescope. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH. SECTION A, ACCELERATORS, SPECTROMETERS, DETECTORS AND ASSOCIATED EQUIPMENT, 596, 100-102 [10.1016/j.nima.2008.07.117].
Low Power Front End for the Optical Module of a Neutrino Underwater Telescope
GIORGI, FILIPPO MARIA;GABRIELLI, ALESSANDRO
2008
Abstract
A proposal for a new system to capture signals in the Optical Module (OM) of an underwater neutrino telescope is described. It concentrates on the problem of power consumption and time precision. In particular, a solution for the interface between the photomultiplier (PMT) and the front-end electronics is presented.File in questo prodotto:
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