| Budget Amount *help |
¥2,600,000 (Direct Cost: ¥2,000,000、Indirect Cost: ¥600,000)
Fiscal Year 2014: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2013: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
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| Outline of Final Research Achievements |
Using the Galactic plane data of Suzaku, I measured the spatial intensity fluctuation of the Galactic ridge X-ray emission (GRXE). I revealed that the combined intensity of the GRXE and cosmic X-ray background fluctuates about 3.6~8.1 % (1 sigma) over about 10 pc, except for systematic errors. This fluctuation is consistent with the prediction of the case that the GRXE is the superposition of many faint point sources.
I also studied the spatial profile of the highly ionized iron line intensity ratio over a few hundred pc. It suggests that the origin of the GRXE possibly differs in the disk and bulge regions.
Based on these studies, I also developed an educational material for high school students to study the Bohr model using Suzaku data.
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