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Titlebook: Large-Scale Structures in the Universe Observational and Analytical Methods; Proceedings of a Wor W. C. Seitter,H. W. Duerbeck,M. Tacke Con

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樓主: T-Lymphocyte
51#
發(fā)表于 2025-3-30 09:02:24 | 只看該作者
52#
發(fā)表于 2025-3-30 15:15:00 | 只看該作者
53#
發(fā)表于 2025-3-30 19:30:50 | 只看該作者
54#
發(fā)表于 2025-3-30 21:55:58 | 只看該作者
55#
發(fā)表于 2025-3-31 03:25:20 | 只看該作者
0075-8450 ional and theoretical approaches to the large scale structures in the universe. The contributions are written with an emphasis on methods. The volume contains among many other topics recent observational results on redshift surveys of clusters and distributions of galaxies and quasars, together with
56#
發(fā)表于 2025-3-31 06:23:41 | 只看該作者
The Edinburgh/Durham galaxy survey,ata reduction techniques for both image classification and image photometry. Preliminary results are presented, including maps of galaxy distribution, together with number-magnitude counts and the galaxy-galaxy correlation function.
57#
發(fā)表于 2025-3-31 12:19:08 | 只看該作者
The Muenster redshift project. Automated redshift measurements from low-dispersion objective prism e majority of cases two . measurements are possible leading to mean redshift values with errors of 0.008. To date redshifts of 24 000 galaxies with 17. < m. < 20. have been obtained. The current rate is an increase of 6 000 galaxy redshifts per measuring week.
58#
發(fā)表于 2025-3-31 15:00:32 | 只看該作者
Conference proceedings 1988on the importance of these findings for future standards and for theoretical predictions. A long historical chapter serves as an introduction. This mixture of textbook and review is aimed at the newcomer to the field as well as at the specialist. Graduate students will find it useful for additional reading.
59#
發(fā)表于 2025-3-31 21:20:05 | 只看該作者
60#
發(fā)表于 2025-4-1 00:09:39 | 只看該作者
The Muenster Redshift project. Automated analysis of galaxy clustering on Schmidt plates,ps of two-dimensional galaxy distributions are presented, including the distributions of different types of galaxies (using ellipticity as a coarse morphological criterion). We present preliminary results for a region near the South Galactic Pole, containing several clusters of galaxies, of which five form a physical group at redshift . = 0.11.
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