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首页> 外文会议>Conference on Survey and Other Telescope Technologies and Discoveries; Aug 27-28, 2002; Waikoloa, Hawaii, USA >Science Breakthroughs with the Sloan Digital Sky Survey: Results and Opportunities
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Science Breakthroughs with the Sloan Digital Sky Survey: Results and Opportunities

机译：斯隆数字天空调查的科学突破：成果与机遇

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摘要

The Sloan Digital Sky Survey represents a new paradigm for optical astronomy. It is a consortium involving several hundred astronomers from the US, Japan, and Germany, and aims to obtain basic photometric and spectroscopic data of a large representative region of the high Galactic latitude sky. Using a dedicated wide-field 2.5m telescope and unique instrumentation and software, it is imaging the sky in five photometric bands, and obtaining high-quality spectra of magnitude-limited samples of galaxies and quasars. Although the original survey goals are oriented towards large-scale structure studies, the survey is yielding major results in fields ranging from high-redshift quasars to Galactic structure, from studies of galaxy properties to asteroids, from brown dwarfs to fluctuations in the Earth's atmosphere. I will give a broad overview of some of these results and give thoughts on some of the types of results we can look forward to in the future of the survey.
机译：Sloan Digital Sky Survey代表了光学天文学的新范例。它是一个由来自美国，日本和德国的数百名天文学家组成的财团，旨在获取高银河纬度天空的大型代表区域的基本光度和光谱数据。使用专用的2.5m宽视场望远镜和独特的仪器和软件，它可以在五个光度学带上对天空进行成像，并获得星系和类星体受幅度限制的样本的高质量光谱。尽管最初的调查目标是针对大规模结构研究，但该调查在从高红移类星体到银河结构，从银河性质到小行星的研究，从棕矮星到地球大气波动的各个领域都取得了重大成果。我将对其中一些结果进行广泛的概述，并对我们将来可以期待的一些结果类型进行思考。

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