Monday Plenary:
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16 - 21 June 2024
Yokohama, Japan
Conference 13093 > Paper 13093-300
Paper 13093-300

Prototype fine-imaging narrow field of view semiconductor Compton telescope with shielded coded-mask, mini-SGI

On demand | Presenting live 19 June 2024

Abstract

Semiconductor Compton telescope (SCT) is one of the promising technologies in cosmic MeV gamma-ray observation, because of good angular resolution measure thanks to its high energy and positional resolutions. However, it cannot be better than a few degrees because of quantum limitation. With improving sensitivity in MeV astronomy, realization of 10-arcmin-level of angular resolution is the essential. Since the mask made of heavy metal is a BGD source and the strong CXB limits the statistical significance of the mask decoding, we propose to adopt this concept on a narrow field of view Si/CdTe SCT, like the SGD onboard ASTRO-H mission. We developed a concept verification system, mini-SGI, adopting 0.5 mm thick DSSDs and 2 mm thick CdTe-DSD, covered with BGO active shield. We irradiated gamma-rays and verified the coded-mask and Compton reconstruction combined analysis.

Presenter

Keigo Okuma
Nagoya Univ. (Japan)
Keigo Okuma is a Ph.D. student at Nagoya University. His work focuses on the development and evaluation of MeV gamma-ray detectors for high-energy astrophysics, and observational study of on-ground thunderstorm gamma-ray observations. He uses CdTe double-sided strip detectors and DSSDs, as well as scintillation detectors. He is also a COSI team member.
Presenter/Author
Keigo Okuma
Nagoya Univ. (Japan)
Author
Kazuhiro Nakazawa
Nagoya Univ. (Japan)
Author
The Univ. of Tokyo (Japan)
Author
Nagoya Univ. (Japan)
Author
Nagoya Univ. (Japan)
Author
Nagoya Univ. (Japan)
Author
Nagoya Univ. (Japan)
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Nagoya Univ. (Japan)
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Japan Aerospace Exploration Agency (Japan)
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The Univ. of Tokyo (Japan)
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Nagoya Univ. (Japan)
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Naoki Ishida
Technical Ctr. of Nagoya Univ. (Japan)
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Takahiro Minami
The Univ. of Tokyo (Japan)
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iMAGINE-X Inc. (Japan)
Author
iMAGINE-X Inc. (Japan)