TL;DR
This paper discusses the development of a Silicon Strip Detector-based Semiconductor Multiple-Compton Telescope for gamma-ray astronomy, emphasizing its high energy resolution and polarization sensitivity.
Contribution
It introduces prototype modules of a low noise DSSD system with significant energy resolution and demonstrates gamma-ray imaging capabilities.
Findings
Achieved 1.3 keV energy resolution at 122 keV
Developed prototype modules for SMCT
Demonstrated gamma-ray imaging test results
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.