Co-Investigator(Kenkyū-buntansha) |
岩田 生 国立天文台, TMTプロジェクト, 准教授 (40399275)
小山 佑世 国立天文台, ハワイ観測所, 准教授 (40724662)
高遠 徳尚 国立天文台, ハワイ観測所, 教授 (50261152)
有本 信雄 国立天文台, ハワイ観測所, 名誉教授 (60242096)
美濃和 陽典 国立天文台, ハワイ観測所, 准教授 (60450194)
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Budget Amount *help |
¥209,690,000 (Direct Cost: ¥161,300,000、Indirect Cost: ¥48,390,000)
Fiscal Year 2021: ¥14,040,000 (Direct Cost: ¥10,800,000、Indirect Cost: ¥3,240,000)
Fiscal Year 2020: ¥14,040,000 (Direct Cost: ¥10,800,000、Indirect Cost: ¥3,240,000)
Fiscal Year 2019: ¥67,860,000 (Direct Cost: ¥52,200,000、Indirect Cost: ¥15,660,000)
Fiscal Year 2018: ¥66,690,000 (Direct Cost: ¥51,300,000、Indirect Cost: ¥15,390,000)
Fiscal Year 2017: ¥47,060,000 (Direct Cost: ¥36,200,000、Indirect Cost: ¥10,860,000)
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Outline of Final Research Achievements |
We conducted research and development of a laser tomography adaptive optics system with multiple laser guide stars. Tomographic estimation of the three dimensional structure of the atmospheric turbulence is demonstrated with a tomographic wavefront sensing unit consists of multiple wavefront sensors. Generation and the science operation of the high brightness laser guide star are conducted successfully with a new fiber laser light source. To reveal the cosmological evolution of structures of disk galaxies, spatially-resolved spectral energy distribution analysis is conducted with high spatial resolution imaging data of distant galaxies, the results indicate that large radial transfer of stellar mass is not necessary to reproduce the structural evolution of the disk galaxies. We developed a code to conduct analysis of combined datasets of high spatial resolution integral field spectroscopy and imaging.
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