Galaxy classification using fractal signature

被引:22
作者
Lekshmi, S
Revathy, K
Nayar, SRP [1 ]
机构
[1] Univ Kerala, Dept Phys, Trivandrum 695581, Kerala, India
[2] Univ Kerala, Dept Comp Sci, Trivandrum 695581, Kerala, India
关键词
galaxies : fundamental parameters (classification); techniques : image processing; methods : data analysis;
D O I
10.1051/0004-6361:20030541
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Fractal geometry is becoming increasingly important in the study of image characteristics. For recognition of regions and objects in natural scenes, there is always a need for features that are invariant and they provide a good set of descriptive values for the region. There are many fractal features that can be generated from an image. In this paper, fractal signatures of nearby galaxies are studied with the aim of classifying them. The fractal signature over a range of scales proved to be an efficient feature set with good discriminating power. Classifiers were designed using nearest neighbour method and neural network technique. Using the nearest distance approach, classification rate was found to be 92%. By the neural network method it has been found to increase to 95%.
引用
收藏
页码:1163 / 1167
页数:5
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