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Proceedings Paper

Development and performance of a gamma-ray imaging detector
Author(s): J. L. Gálvez; M. Hernanz; J. M. Álvarez; M. La Torre; L. Álvarez; D. Karelin; M. Lozano; G. Pellegrini; M. Ullán; E. Cabruja; R. Martínez; M. Chmeissani; C. Puigdengoles
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Paper Abstract

In the last few years we have been working on feasibility studies of future instruments in the gamma-ray range, from several keV up to a few MeV. The innovative concept of focusing gamma-ray telescopes in this energy range, should allow reaching unprecedented sensitivities and angular resolution, thanks to the decoupling of collecting area and detector volume. High sensitivities are essential to perform detailed studies of cosmic explosions and cosmic accelerators, e.g., Supernovae, Classical Novae, Supernova Remnants (SNRs), Gamma-Ray Bursts (GRBs), Pulsars, Active Galactic Nuclei (AGN). In order to achieve the needed performance, a gamma-ray imaging detector with mm spatial resolution and large enough efficiency is required. In order to fulfill the combined requirement of high detection efficiency with good spatial and energy resolution, an initial prototype of a gamma-ray imaging detector based on CdTe pixel detectors is being developed. It consists of a stack of several layers of CdTe detectors with increasing thickness, in order to enhance the gamma-ray absorption in the Compton regime. A CdTe module detector lies in a 11 x 11 pixel detector with a pixel pitch of 1mm attached to the readout chip. Each pixel is bump bonded to a fan-out board made of alumina (Al2O3) substrate and routed to the corresponding input channel of the readout ASIC to measure pixel position and pulse height for each incident gamma-ray photon. We will report the main features of the gamma-ray imaging detector performance such as the energy resolution for a set of radiation sources at different operating temperatures.

Paper Details

Date Published: 17 September 2012
PDF: 12 pages
Proc. SPIE 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, 844336 (17 September 2012); doi: 10.1117/12.925979
Show Author Affiliations
J. L. Gálvez, Institut de Ciències de l’Espai, CSIC-IEEC, Univ. Autònoma de Barcelona (Spain)
M. Hernanz, Institut de Ciències de l’Espai, CSIC-IEEC, Univ. Autònoma de Barcelona (Spain)
J. M. Álvarez, Institut de Ciències de l’Espai, CSIC-IEEC, Univ. Autònoma de Barcelona (Spain)
M. La Torre, Institut de Ciències de l’Espai, CSIC-IEEC, Univ. Autònoma de Barcelona (Spain)
L. Álvarez, Institut de Ciències de l’Espai, CSIC-IEEC, Univ. Autònoma de Barcelona (Spain)
D. Karelin, Institut de Ciències de l’Espai, CSIC-IEEC, Univ. Autònoma de Barcelona (Spain)
M. Lozano, Centro Nacional de Microelectrónica IMB-CNM CSIC, Univ. Autònoma de Barcelona (Spain)
G. Pellegrini, Centro Nacional de Microelectrónica IMB-CNM CSIC, Univ. Autònoma de Barcelona (Spain)
M. Ullán, Centro Nacional de Microelectrónica IMB-CNM CSIC, Univ. Autònoma de Barcelona (Spain)
E. Cabruja, Centro Nacional de Microelectrónica IMB-CNM CSIC, Univ. Autònoma de Barcelona (Spain)
R. Martínez, Centro Nacional de Microelectrónica IMB-CNM CSIC, Univ. Autònoma de Barcelona (Spain)
M. Chmeissani, Institut de Física d’Altes Energies, Univ. Autònoma de Barcelona (Spain)
C. Puigdengoles, Institut de Física d’Altes Energies, Univ. Autònoma de Barcelona (Spain)


Published in SPIE Proceedings Vol. 8443:
Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
Tadayuki Takahashi; Stephen S. Murray; Jan-Willem A. den Herder, Editor(s)

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