| Budget Amount *help |
¥17,160,000 (Direct Cost: ¥13,200,000、Indirect Cost: ¥3,960,000)
Fiscal Year 2023: ¥5,070,000 (Direct Cost: ¥3,900,000、Indirect Cost: ¥1,170,000)
Fiscal Year 2022: ¥5,070,000 (Direct Cost: ¥3,900,000、Indirect Cost: ¥1,170,000)
Fiscal Year 2021: ¥5,070,000 (Direct Cost: ¥3,900,000、Indirect Cost: ¥1,170,000)
Fiscal Year 2020: ¥1,950,000 (Direct Cost: ¥1,500,000、Indirect Cost: ¥450,000)
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| Outline of Final Research Achievements |
By systematically analyzing the multi-wavelength data of ultra/luminous infrared galaxies in the local Universe, we have revealed that the galaxies and supermassive black holes in their centers "co-evolve" by galaxy mergers, where AGN feedback works in the later stage. We have suggested the possibility that heavily obscured AGNs in similar populations at the more distant Universe may be missed in the current X-ray surveys. Comparing the AGN and host galaxy properties between high luminosity AGNs at z~1.5 and low luminosity ones at z=0.2-0.8, we find no evidence that their formation processes are different. We have proposed a new unified model of AGN by including polar dusty gas, in order to consistently explain the infrared and X-ray spectra of local AGNs.
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