| 研究課題/領域番号 |
21F21325
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| 配分区分 | 補助金 |
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| 研究機関 | 東京大学 |
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研究代表者 |
SILVERMAN John 東京大学, カブリ数物連携宇宙研究機構, 教授 (90573030)
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| 研究分担者 |
YANG LILAN 東京大学, カブリ数物連携宇宙研究機構, 外国人特別研究員
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| 研究期間 (年度) |
2021-11-18 – 2024-03-31
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| キーワード | galaxy formation / gravitational waves / JWST |
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| 研究実績の概要 |
I have used the JSPS Grant-in-Aid to support research on the size-luminosity scaling relation of bright galaxies in the early Universe (i.e., reionization epoch), and understand the mass distribution of the black hole mass-based gravitational wave data. I performed the analysis using the observation data based on the brand-new space telescope JWST. The data is from one of the early release science projects of JWST, and enable us to probe the high redshift galaxy’s morphology and scaling relation for the first time. We found that the size of high redshift galaxies does not vary significantly as a function of wavelength, i.e., from rest-frame UV to optical. We also detected a tentative steeper slope of size-luminosity relation at the rest-frame UV band which indicates that the faint galaxies have extremely small sizes. Furthermore, I also investigated the impact of gravitational lensing on the black hole mass distribution function, and found the current influence from lensing is insignificant. In summary, my main research outcome is the first study of rest-frame optical size-luminosity relation at z>7, and it has made significant contributions understand the galaxy’s morphology and scaling relation in early Universe.
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| 現在までの達成度 (区分) |
現在までの達成度 (区分)
2: おおむね順調に進展している
理由
I have made progress over the past year in investigating the size-luminosity scaling relation of bright galaxies in the early Universe and understanding the mass distribution of the black hole mass-based gravitational wave data. With the brand-new telescope, it enables the investigation of the rest-frame optical size-luminosity scaling relation, and I have gained a better understanding of the properties of early galaxies. The outcomes of my research are evidenced by several publications that have resulted from it in FY2022, including morphological properties and the size-luminosity scaling relation of galaxies, and their wavelength dependence. These findings are significant because they improve our knowledge of understanding galaxy formation and evolution, and its properties at the reionization epoch. Additionally, the achievements of the past year have set a strong foundation for my upcoming research activities.
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| 今後の研究の推進方策 |
For the upcoming year, I plan to continue my research effort on studying the properties of galaxies as a function of wavelength at a wide, using a larger data sample, i.e., from the largest JWST survey COSMOS-Web. I will study the properties of fainter galaxies which are magnified by foreground gravitational lenses such as galaxies and clusters. Additionally, I will use the simulations to further understand galaxy formation and evolution, such as making a direct comparison with our observational results to different simulations, which will provide important clues to verify the assumptions adopted in the simulation.
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