| Budget Amount *help |
¥3,380,000 (Direct Cost: ¥2,600,000、Indirect Cost: ¥780,000)
Fiscal Year 2022: ¥520,000 (Direct Cost: ¥400,000、Indirect Cost: ¥120,000)
Fiscal Year 2021: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2020: ¥520,000 (Direct Cost: ¥400,000、Indirect Cost: ¥120,000)
Fiscal Year 2019: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2018: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
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| Outline of Final Research Achievements |
To clarify the links among the properties of ionized gas, dark matter, stars and AGNs in galaxy clusters, we have utilized multi-wavelength astrophysical data and state-of-the-art cosmological numerical simulations. Our main achievements are that we have successfully measured the Sunyaev-Zel'dovich effect from three galaxy clusters at 5 arcsec resolution, verified the presence of a galaxy cluster that hosts a radiative cooling flow, and shown that dipolar perturbations of gas density and temperature are present ubiquitously even in apparently relaxed galaxy clusters.
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