1. Development of a detector based on Silicon Drift Detectors for gamma-ray spectroscopy for astronomy applications
- Author
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Claudio Piemonte, Nicola Zorzi, Paolo Busca, Luca Bombelli, R. Quaglia, Gabriele Giacomini, Angelo Geraci, Carlo Fiorini, Brian Shortt, Maurizio Boscardin, R. Peloso, S. Incorvaia, P. Bellutti, Francesco Ficorella, Nick Nelms, and A. Picciotto
- Subjects
Physics ,sezele ,Silicon ,business.industry ,Detector ,Gamma ray ,chemistry.chemical_element ,Astronomy ,Scintillator ,Semiconductor detector ,Optics ,chemistry ,Optoelectronics ,Gamma spectroscopy ,Quantum efficiency ,business ,Spectroscopy - Abstract
This work deals with the development of a new gamma detector based on Silicon Drift Detectors (SDDs) to read out large (3"×3") LaBr3:Ce scintillators for gamma-ray spectroscopy for astronomy applications, an activity supported by European Space Agency (ESA). SDDs, characterized by high quantum efficiency and low electronic noise, are good candidates in applications with a wide energy range of gamma rays to be detected from 150keV to 15MeV. A first prototype is under development with the aim to achieve an energy resolution of 3% FWHM at 662 keY. The SDDs are designed as monolithic arrays of 3×3 units, each one of an active area of 8 mm × 8 mm (total array area of 26 mm × 26 mm).To cover the large surface of the 3"×3" LaBr3:Ce scintillator the modules are expected to be arranged in a 3×3 matrix, for a total of 81 SDDs read out by a custom developed electronics. In this work we will report on the design issues of this detector and on the first experimental results obtained in gamma-ray spectroscopy with a 1"×1" LaBr3:Ce scintillator.
- Published
- 2012