Celestial MeV gamma-ray observation using electron-tracking Compton camera loaded on long duration balloons (SMILE-3)

MeV gamma-ray observations provide unique information about nucleosynthesis, diffusion in our galaxy, low-energy cosmic rays, particle acceleration, and other phenomena. However, the detection sensitivity in this band is significantly lower than that in other bands due to a large background contamination. To address this issue, we are developing an electron-tracking Compton camera (ETCC) with powerful background rejection tools based on Compton recoil electron tracks. This will enable future observations to be conducted with greater sensitivity. We have successfully demonstrated the detection technology and performance of the ETCC with two balloon experiments. We are preparing for the next balloon flight, SMILE-3, to observe galactic diffusion gamma rays and some bright celestial objects.

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Published
2024-08-21
DOI
https://doi.org/10.1117/12.3016872
Primary Topic
Particle Detector Development and Performance
Type
article
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article

Celestial MeV gamma-ray observation using electron-tracking Compton camera loaded on long duration balloons (SMILE-3)

K. Miuchi, M. Mori, Yoshitaka Mizumura, Tomonori Ikeda et al.
Particle Detector Development and Performance
article

Celestial MeV gamma-ray observation using electron-tracking Compton camera loaded on long duration balloons (SMILE-3)

K. Miuchi, M. Mori, Yoshitaka Mizumura, Tomonori Ikeda, Atsushi Takada, Shunsuke Kurosawa, Kenji Hamaguchi, Mitsuru Abe, Takeshi Nakamori, Hirotake Tsukamoto, Tomohiko Oka, T. Tanimori, Tatsuya Sawano, J. Kushida, Haruki Iiyama, Kei Yoshikawa, Ryo Yoshioka, Taito Takemura
article en

Abstract

MeV gamma-ray observations provide unique information about nucleosynthesis, diffusion in our galaxy, low-energy cosmic rays, particle acceleration, and other phenomena. However, the detection sensitivity in this band is significantly lower than that in other bands due to a large background contamination. To address this issue, we are developing an electron-tracking Compton camera (ETCC) with powerful background rejection tools based on Compton recoil electron tracks. This will enable future observations to be conducted with greater sensitivity. We have successfully demonstrated the detection technology and performance of the ETCC with two balloon experiments. We are preparing for the next balloon flight, SMILE-3, to observe galactic diffusion gamma rays and some bright celestial objects.

Vol. 930
Kanazawa University (JP), Yamagata University (JP), Tokai University (JP), Ritsumeikan University (JP), Tohoku University (JP), Kyoto University (JP), Japan Aerospace Exploration Agency (JP), Institute of Space and Astronautical Science (JP), Kobe University (JP), University of Maryland, Baltimore County (US)
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Openalex Percentile: Top 96%
Particle Detector Development and Performance
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