| Budget Amount *help |
¥15,080,000 (Direct Cost: ¥11,600,000、Indirect Cost: ¥3,480,000)
Fiscal Year 2014: ¥2,210,000 (Direct Cost: ¥1,700,000、Indirect Cost: ¥510,000)
Fiscal Year 2013: ¥2,860,000 (Direct Cost: ¥2,200,000、Indirect Cost: ¥660,000)
Fiscal Year 2012: ¥2,730,000 (Direct Cost: ¥2,100,000、Indirect Cost: ¥630,000)
Fiscal Year 2011: ¥2,080,000 (Direct Cost: ¥1,600,000、Indirect Cost: ¥480,000)
Fiscal Year 2010: ¥5,200,000 (Direct Cost: ¥4,000,000、Indirect Cost: ¥1,200,000)
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| Outline of Final Research Achievements |
Gamma-Ray Bursts (GRBs) and Active Galactic Nuclei (AGNs) are the two archetypical phenomena among astrophysical jets. This study consists of multi-wavelength observational study of these objects to investigate (A) the life of the jets, (B) physics of radiation region, and (C) circumstances including intergalactic warm-hot plasma. Through this study we realized that: the life time of AGN jets is up to 100 Myears with a fairly constant energy ejection; the radiation of the GRB prompt emission consists both of non-thermal synchrotron and thermal blackbody like emissions. We also developed X-ray micro-calorimeter system for the next generation X-ray observatory ASTRO-H and made observation plan to reveal warm-hot intergalactic medium irradiated by GRB or relativistically beamed AGN jets.
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