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发表于 2025-3-21 17:53:28 | 显示全部楼层 |阅读模式
书目名称Gravitational Lenses
编辑Peter Schneider,Jürgen Ehlers,Emilio E. Falco
视频video
丛书名称Astronomy and Astrophysics Library
图书封面Titlebook: ;
出版日期Book 19921st edition
版次1
doihttps://doi.org/10.1007/978-1-4612-2756-4
isbn_softcover978-1-4612-7655-5
isbn_ebook978-1-4612-2756-4Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
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书目名称Gravitational Lenses影响因子(影响力)




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发表于 2025-3-21 21:49:41 | 显示全部楼层
Statistical gravitational lensing: Applications,The discussion in the preceding chapter focused on the technical aspects of statistical lensing. We now turn to the applications of statistical lensing, making extensive use of the results obtained in Chap. 11.
发表于 2025-3-22 03:03:43 | 显示全部楼层
https://doi.org/10.1007/0-387-28003-0ity of multiple imaging of sources and the magnification and distortion of the shape of images. Detailed knowledge of the properties of simple lens models is essential for the understanding of observed lens cases. In this and the following chapter, we consider the statistical properties of an ensemble of lenses.
发表于 2025-3-22 07:58:44 | 显示全部楼层
发表于 2025-3-22 09:11:21 | 显示全部楼层
发表于 2025-3-22 15:36:54 | 显示全部楼层
Gravitational lenses as astrophysical tools,urnish an additional test of General Relativity; (2.) allow us to see fainter or more distant sources; and (3.) provide a means to estimate the mass of galaxies, of clusters of galaxies, and of unseen, massive aggregates of dark matter.
发表于 2025-3-22 19:41:42 | 显示全部楼层
Gravitational Lenses978-1-4612-2756-4Series ISSN 0941-7834 Series E-ISSN 2196-9698
发表于 2025-3-22 22:33:19 | 显示全部楼层
发表于 2025-3-23 02:18:38 | 显示全部楼层
Numerical methods,ot known a priori. There are other problems where numerical analysis must be applied, e.g., if one wants to determine the total magnification for an extended source, as a function of its position. This problem is computationally simpler than the standard problem.
发表于 2025-3-23 09:00:23 | 显示全部楼层
Basic facts and the observational situation,een images, and who are not interested in the more detailed aspects of gravitational lens theory discussed in later chapters. In particular, a “guide for observers” is presented, concerning the search for, and the detection and verification of GL events. An overview of observed GL candidates is presented in Sect. 2.5.
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