Fuzzy classifier for star-galaxy separation

被引:12
|
作者
Mähönen, P
Frantti, T
机构
[1] Univ Oulu, Dept Phys Sci, FIN-90570 Oulu, Finland
[2] VTT, Tech Res Ctr Finland, FIN-90570 Oulu, Finland
[3] VTT, Tech Res Ctr Finland, Networking Res, FIN-90571 Oulu, Finland
来源
ASTROPHYSICAL JOURNAL | 2000年 / 541卷 / 01期
关键词
methods : data analysis; methods : numerical; techniques : image processing;
D O I
10.1086/309424
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The sizes of astronomical surveys are increasing rapidly. Hence, the automatic classification of objects is growing more important. This classification is traditionally based, e.g., on point-spread function fitting. Recently several different neural network. approaches have been introduced. In this paper we introduce a simple method that is based on fuzzy set reasoning. The analysis presented here concentrates on separating point sources (stars) from extended ones. The tests show that the neural network approach is superior if compared to direct fuzzy classification. The paper shows that the inherent ability of neural networks to process complex nonlinear data justifies the use of them in astronomical classification However, a combined fuzzy and neural network approach can be useful at least in special cases.
引用
收藏
页码:261 / 263
页数:3
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