| Budget Amount *help |
¥413,270,000 (Direct Cost: ¥317,900,000、Indirect Cost: ¥95,370,000)
Fiscal Year 2019: ¥69,420,000 (Direct Cost: ¥53,400,000、Indirect Cost: ¥16,020,000)
Fiscal Year 2018: ¥53,300,000 (Direct Cost: ¥41,000,000、Indirect Cost: ¥12,300,000)
Fiscal Year 2017: ¥73,840,000 (Direct Cost: ¥56,800,000、Indirect Cost: ¥17,040,000)
Fiscal Year 2016: ¥90,480,000 (Direct Cost: ¥69,600,000、Indirect Cost: ¥20,880,000)
Fiscal Year 2015: ¥126,230,000 (Direct Cost: ¥97,100,000、Indirect Cost: ¥29,130,000)
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| Outline of Final Research Achievements |
We developed a cosmological analysis method that can be done by combining weak lensing information and galaxy clustering that are observed from wide-field imaging galaxy survey and spectroscopic surveys, respectively. In particular, we developed Dark Emulator that allows for fast, accurate computations of cosmological clustering quantities, using about 300TB data of N-body simulations based on machine learning. In addition, we constructed the near-infrared spectrograph camera for the Subaru Prime Focus Spectrograph project, working together with researchers from Princeton University and Johns Hopkins University.
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