| Budget Amount *help |
¥4,160,000 (Direct Cost: ¥3,200,000、Indirect Cost: ¥960,000)
Fiscal Year 2013: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2012: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2011: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2010: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
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| Research Abstract |
In order to clarify the mechanism of high-energy gamma-ray emission from celestial active objects, we analyzed the gamma-ray data observed by the LAT detector onboard the Fermi Gamma-ray Space Telescope.
Especially Galactic objects, like X-ray binaries, supernova remnants and pulsar nebula are the main targets of this study. We detected the gamma-ray signal from an X-ray binary and a pulsar nebula, PSR1259-63/SS2883, when it passed the periastron in 2010 December. We also gave upper limits on gamma-ray emission from seven X-ray binaries. Other objects are under analysis.
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