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Development of a Gamma-ray Burst Detector Based on the Silicon Drift Detector Array and Scintillators

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.2943548· OSTI ID:21137230
; ; ; ; ; ; ;  [1];  [2]; ;  [3];  [4];  [5]
  1. Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 229-8558 (Japan)
  2. KETEK GmbH, Hofer Strasse 3, 81737 Munchen (Germany)
  3. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510 (Japan)
  4. Clear Pulse Ltd, 6-25-17 Chuoh, Ohta-ku, Tokyo 143-0024 (Japan)
  5. Makishima Cosmic Radiation Laboratory, Institute of Physical and Chemical Research (RIKEN), 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan)
We propose a gamma-ray burst (GRB) detector combining the silicon drift detector (SDD) array and scintillators with broadband X-ray and gamma-ray coverage (0.5-1000 keV or more), high energy resolution (2-10%) and high time resolution ({approx}{mu}s) in space. To realize such compact high-performance detector without photomultiplier tubes, we constructed proto-type model using KETEK SDD with a detection area of 1 cm{sup 2} and BGO crystal. The detector shows a very good performance. Obtained FWHM energy resolution was 191 eV at 5.9 keV in the SDD, while 6.5 % at 662 keV in the BGO at -30 deg. C. Evaluation of the 7 channel SDD array and development of analog ASIC for its readout are also presented.
OSTI ID:
21137230
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1000; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English