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Titlebook: Rough Sets and Knowledge Technology; 4th International Co Peng Wen,Yuefeng Li,Guoyin Wang Conference proceedings 2009 Springer-Verlag Berli

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樓主: interminable
31#
發(fā)表于 2025-3-27 00:20:26 | 只看該作者
32#
發(fā)表于 2025-3-27 02:06:33 | 只看該作者
Improving Rules Quality Generated by Rough Set Theory for the Diagnosis of Students with LDs througherforms better in term of prediction certainty than other rule-based algorithms such as decision tree and ripper algorithms. Overall, we believe that RST may have the potential in playing an essential role in the field of LD diagnosis.
33#
發(fā)表于 2025-3-27 05:56:35 | 只看該作者
34#
發(fā)表于 2025-3-27 12:10:02 | 只看該作者
d to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e?ciency, so that far more than the observed fraction of about 10–15% of the baryonic matter would be found in lu
35#
發(fā)表于 2025-3-27 15:53:03 | 只看該作者
Andrzej Jankowski,Andrzej Skowron,Marcin Szczukad to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e?ciency, so that far more than the observed fraction of about 10–15% of the baryonic matter would be found in lu
36#
發(fā)表于 2025-3-27 20:43:22 | 只看該作者
David M. W. Powers,Richard Leibbrandtd to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e?ciency, so that far more than the observed fraction of about 10–15% of the baryonic matter would be found in lu
37#
發(fā)表于 2025-3-28 00:43:16 | 只看該作者
38#
發(fā)表于 2025-3-28 03:26:53 | 只看該作者
39#
發(fā)表于 2025-3-28 09:58:20 | 只看該作者
Rafael Falcón,Gwanggil Jeon,Kangjun Lee,Rafael Bello,J. Jeongthe gaseous baryons did not cool, collapse, and form stars and galaxies. However, if this gas is allowed to cool unimpeded at the rate predicted from known atomic physics, in the context of a well-established cosmological model, the gaseous matter would form stars and galaxies with a high e?ciency,
40#
發(fā)表于 2025-3-28 12:44:59 | 只看該作者
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