| Project/Area Number |
22540245
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| Research Category |
Grant-in-Aid for Scientific Research (C)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Astronomy
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| Research Institution | The University of Tokyo |
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Principal Investigator |
KAMAE Tuneyoshi 東京大学, 大学院・理学系研究科, 名誉教授 (90011618)
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| Co-Investigator(Renkei-kenkyūsha) |
MAKISHIMA Kazuo 東京大学, 大学院・理学系研究科, 教授 (20126163)
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| Project Period (FY) |
2010 – 2012
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| Project Status |
Completed (Fiscal Year 2012)
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| Budget Amount *help |
¥4,290,000 (Direct Cost: ¥3,300,000、Indirect Cost: ¥990,000)
Fiscal Year 2012: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2011: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2010: ¥2,340,000 (Direct Cost: ¥1,800,000、Indirect Cost: ¥540,000)
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| Keywords | 気球実験 / 軟ガンマ線偏光検出器 / かに星雲 / 白鳥座 / ブラックホール |
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| Research Abstract |
The aim of the research program has been to mount the hard X-ray polarimeter (PoGOLite) we produced with other funds onto a gondola in ESRANGE balloon station in Sweden, and to carry out one-week-long observations of Crab Nebula and Cygnus X-1 onboard a balloon. The polarimeter, control system, and gondola assembly have been built on funds and grants from Stanford Univ., Wallenberg Foundation, JSPS and Swedish Space Board. Two possible long-duration flight routes have been considered: the shorter one is one-week-long flight from Sweden to northern Canada and the longer one is three-week-long circumnavigation around the North Pole. The polarimeter is most sensitive between 20keV and 60keV and capable of detecting 3% polarization in the energy band for Crab Nebula and Cyg X-1 in the hard state. Successful detection of polarization in the targets in the energy range will unravel the emission mechanism and the orientation of the magnetic field at the hard X-ray sources. So far no high accuracy measurement has been made in the energy range. The funds will be used to support Japanese collaboration members to participate in the balloon flight and data analyses.
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