| Budget Amount *help |
¥43,420,000 (Direct Cost: ¥33,400,000、Indirect Cost: ¥10,020,000)
Fiscal Year 2022: ¥7,540,000 (Direct Cost: ¥5,800,000、Indirect Cost: ¥1,740,000)
Fiscal Year 2021: ¥7,410,000 (Direct Cost: ¥5,700,000、Indirect Cost: ¥1,710,000)
Fiscal Year 2020: ¥8,840,000 (Direct Cost: ¥6,800,000、Indirect Cost: ¥2,040,000)
Fiscal Year 2019: ¥8,970,000 (Direct Cost: ¥6,900,000、Indirect Cost: ¥2,070,000)
Fiscal Year 2018: ¥10,660,000 (Direct Cost: ¥8,200,000、Indirect Cost: ¥2,460,000)
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| Outline of Final Research Achievements |
A ground-based telescope system (H.E.S.S. Imaging Atmospheric Cherenkov Telescopes) was used to observe very-high-energy gamma rays emitted by celestial bodies that accelerate cosmic rays. Combining X-ray and gamma-ray observations from space with the Chandra X-ray Satellite and the Fermi Gamma-ray Space Telescope, we performed multi-wavelength observations of cosmic-ray accelerators.
We have obtained observational results such as the detection of small gamma-ray flares from the Crab Nebula and detailed measurements of the spatial structure of gamma-ray emissions from supernova remnants. In addition to research results on the kinetics of supernova explosions, we have also obtained results on similarities in temporal variations between X-rays and very-high-energy gamma-rays in the afterglow of a gamma-ray burst.
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