| Budget Amount *help |
¥44,460,000 (Direct Cost: ¥34,200,000、Indirect Cost: ¥10,260,000)
Fiscal Year 2020: ¥9,620,000 (Direct Cost: ¥7,400,000、Indirect Cost: ¥2,220,000)
Fiscal Year 2019: ¥9,490,000 (Direct Cost: ¥7,300,000、Indirect Cost: ¥2,190,000)
Fiscal Year 2018: ¥9,490,000 (Direct Cost: ¥7,300,000、Indirect Cost: ¥2,190,000)
Fiscal Year 2017: ¥8,970,000 (Direct Cost: ¥6,900,000、Indirect Cost: ¥2,070,000)
Fiscal Year 2016: ¥6,890,000 (Direct Cost: ¥5,300,000、Indirect Cost: ¥1,590,000)
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| Outline of Final Research Achievements |
In order to understand the co-evolution between galaxies and intergalactic matter during the course of the cosmic time, quasar absorption line systems found in ultraviolet spectra of quasars provide useful observational tools to investigate the co-evolution. Using ALMA (Atacama Large Millimeter Array) and the Subaru Telescope (8.2 m optical/infrared telescope at Mauna Kea Observatory in Hawaii), we have studied both high redshift starburst/superwind galaxies and extended intergalactic ionized gas clouds, Using these studies, we have obtained important observational constraints on the early evolution of galaxies at high redshift. We have also found firm evidence for a binary supermassive black hole in the nearby AGN, NGC 1068. This discovery reinforces the importance of galaxy mergers in the formation of AGN.
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