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arXiv · hep-ex/0302008

Gamma-ray Polarimetry

Hiroyasu Tajima
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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.

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Hiroyasu Tajima. 2003-02-07. Gamma-ray Polarimetry. https://doi.org/10.1016/s0168-9002(03)01808-4

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