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Gamma-ray polarimetry

Name: Gamma-ray polarimetry
Creator: Hiroyasu Tajima
Keywords: High Energy Physics - Experiment (hep-ex), 03 medical and health sciences, 0302 clinical medicine, Astrophysics (astro-ph), 0103 physical sciences, FOS: Physical sciences, Astrophysics, 01 natural sciences, High Energy Physics - Experiment

descriptionPublicationkeyboard_double_arrow_right Article , Report , Preprint , Other literature type 05 Feb 2003Embargo end date: 01 Jan 2003 English Publisher:Elsevier BVJournal:Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, volume 511, pages 287-290 (issn: 0168-9002,

Authors: Hiroyasu Tajima;

doi: 10.1016/s0168-9002(03)01808-4 , 10.2172/812632 , 10.48550/arxiv.hep-ex/0302008

arXiv: http://arxiv.org/abs/hep-ex/0302008

Gamma-ray polarimetry

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Abstract

An astrophysics application of a low noise Double-sided Silicon Strip Detector (DSSD) is described. A Semiconductor Multiple-Compton Telescope (SMCT) is being developed to explore the gamma-ray universe in the 0.1-20 MeV energy band. Excellent energy resolution and polarization sensitivity are key features of the SMCT. We have developed prototype modules for a low noise DSSD system, which reached an energy resolution of 1.3 keV (FWHM) for 122 keV at 0 degree C. Results of a gamma-ray imaging test are also presented.

6 pages, 9 figures. Contributed to International Workshop on Vertex Detectors, Kailua-Kona, Hawaii USA, November 3-8, 2002

Related Organizations

SLAC National Accelerator Laboratory
United States
Stanford University
United States
Hiroshima University
Japan
College of New Jersey
United States
Stanford University
United States

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Keywords

High Energy Physics - Experiment (hep-ex), Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics, High Energy Physics - Experiment

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