| Project/Area Number |
15204011
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| Research Category |
Grant-in-Aid for Scientific Research (A)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Astronomy
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| Research Institution | The University of Tokyo |
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Principal Investigator |
FUKUGITA Masataka The University of Tokyo, Institute for Cosmic Ray Research, Professor (40100820)
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| Co-Investigator(Kenkyū-buntansha) |
OKAMURA Sadanori The University of Tokyo, Graduate School of Science, Professor (20114423)
YASUDA Naoki The University of Tokyo, Institute for Cosmic Ray Research, Associate Professor (80333277)
ICHIKAWA Shinichi NAOJ, Astronomical data archives center, Associate Professor (80211738)
DOI Manoru The University of Tokyo, Graduate School of Science, Associate Professor (00242090)
SUTOU Yasushi The University of Tokyo, Graduate School of Science, Professor (20206569)
市川 隆 東北大学, 理学部, 助教授 (80212992)
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| Project Period (FY) |
2003 – 2006
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| Project Status |
Completed (Fiscal Year 2006)
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| Budget Amount *help |
¥50,310,000 (Direct Cost: ¥38,700,000、Indirect Cost: ¥11,610,000)
Fiscal Year 2006: ¥12,350,000 (Direct Cost: ¥9,500,000、Indirect Cost: ¥2,850,000)
Fiscal Year 2005: ¥12,350,000 (Direct Cost: ¥9,500,000、Indirect Cost: ¥2,850,000)
Fiscal Year 2004: ¥12,350,000 (Direct Cost: ¥9,500,000、Indirect Cost: ¥2,850,000)
Fiscal Year 2003: ¥13,260,000 (Direct Cost: ¥10,200,000、Indirect Cost: ¥3,060,000)
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| Keywords | SDSS / Galaxy Observations / Large-Scale Astronomical Catalogue / Baryon Acoustic Oscillation / Large-Scale Structure of the Universe / High-Redshift Quasars / Luminosity Functions / Morphological Classification of Galaxies / 銀河觀測(測光掃天、分光觀測) / 天髄型録(銀河、準星) / Sloan Digital Sky Survey / SDSS型録 / 銀河のパワースペクトル / 宇宙論パラメター / CDM模型 / 銀河の光度重元素相関 / 宇宙エネルギー目録 / 宇宙定數 / 楕円銀河 / 星生成 / 重力レンズ / 測光較正 |
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| Research Abstract |
The SDSS project finished its originally planned operations in June 2005. We began the construction of the instruments in 1993 and the operation in 2000. During the time it attained imaging for 115% of the planned region and spectroscopy for 76%. Somewhat lower achievement of the spectroscopy is due to poor weather in the winter and spring of 2004 and 2005. We began a new programme, SDSS-II for another three years from July 2005, for the purpose primarily to fill the missing observed regions, supplemented with two new projects, for which SDSS turns out to be extremely useful from our experience.
To date we have made public the imaging data for 6670 square degrees that comprises 180 million astronomical objects, a half of them being galaxies, and spectra of 850 thousand galaxies. The present Grant-in-Aid project corresponds to the mid to the latest part of the original project and SDSS-II.
Analyses of the acquired data were made from time to time, and our achievements have already satisfied well the scientific goals set in the beginning of the project. The data we acquired are and will be used world-widely throughout this century for precision astronomical sciences. The SDSS project is regarded as the most successful scientific project in our time. The members of the Grant-in-Aid authored 108 papers that have already received over 16000 citations in the community.
The science produced ranges from cosmology, large-scale structure of the universe, high redshift quasars and studies for high redshift universe, galactic astronomy, stellar science, especially that of low temperature stars, and asteroid science. Probably the most important is the quantitative verification that our universe and its evolution are described well by the model of the universe dominated by cold dark matter and dark energy. This allowed our basic understanding of the Universe. The result also indicates the direction and objectives to be studied with large-scale astronomical projects in the future.
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