| Project/Area Number |
20340042
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| Research Category |
Grant-in-Aid for Scientific Research (B)
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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 |
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| Co-Investigator(Renkei-kenkyūsha) |
MOTOHARA Kentaro 東京大学, 理学系研究科, 准教授 (90343102)
AOKI Wako 国立天文台, 助教 (20321581)
NOGUCHI Kunio 国立天文台, 教授 (10111824)
MINOWA Yosuke 国立天文台, 研究員 (60450194)
TSUJIMOTO Takuji 国立天文台, 助教 (10270456)
KAWABATA Koji 広島大学, 宇宙科学センター, 准教授 (60372702)
KAWAKITA Hideyo 京都産業大学, 理学部, 教授 (70356129)
OKOSHI Katsuya 東京理科大学, 基礎工学部, 講師 (50453832)
NAGASHIMA Masahiro 長崎大学, 教育学部, 准教授 (20342628)
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| Research Collaborator |
IKEDA Yuji 京都産業大学, 理学部, 准教授 (40550611)
KONDO Sohei 京都産業大学, 神山天文台, 特定研究員(PD) (30583413)
YASUI Chikako 国立天文台, 研究員 (00583626)
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| Project Period (FY) |
2008 – 2010
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| Project Status |
Completed (Fiscal Year 2010)
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| Budget Amount *help |
¥19,500,000 (Direct Cost: ¥15,000,000、Indirect Cost: ¥4,500,000)
Fiscal Year 2010: ¥3,380,000 (Direct Cost: ¥2,600,000、Indirect Cost: ¥780,000)
Fiscal Year 2009: ¥7,280,000 (Direct Cost: ¥5,600,000、Indirect Cost: ¥1,680,000)
Fiscal Year 2008: ¥8,840,000 (Direct Cost: ¥6,800,000、Indirect Cost: ¥2,040,000)
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| Keywords | 高分散分光 / 赤外線 / 近赤外線 / イマージョングレーティング / ガンマ線バースト / クェーサー吸収線系 / 銀河間物質 / 宇宙再電離 / 低金属量 / 恒星 |
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| Research Abstract |
We have developed a next-generation near-infrared high-resolution spectrograph "WINERED", which enables high-sensitive absorption spectroscopy of intergalactic medium in the re-ionization era. WINERED achieves a high-resolution of R=30, 000 despite its compact design and a high throughput that doubles that for conventional high-resolution spectrographs by narrowing the wavelength coverage(0. 9-1. 4um) and by using non-cryogenic optics. After completing the assembly and laboratory experiments, we started astronomical observations with the 1. 3m telescope of Koyama Astronomical Observatory at Kyoto Sangyo University. We also experimentally constructed an observational scheme for the follow-up of gamma-ray bursts.
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