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Titlebook: Computer Analysis of Images and Patterns; 16th International C George Azzopardi,Nicolai Petkov Conference proceedings 2015 Springer Interna

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,Sur le problème de levi banachique,g size and Hu’s and Flusser’s image invariant moments information is computed for every segmented galaxy. The C4.5 tree classifier with bagging gives the best classification result. Mergers and projected galaxies are classified with a precision of about 80%.
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https://doi.org/10.1007/BFb0077395lues, and removes them from the MAP estimation by incorporating the weights of pixels into the likelihood term. We conducted a number of experiments using both real and synthetic images, and qualitatively and quantitatively confirmed that our method works better than the existing methods.
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https://doi.org/10.1007/BFb0077395r of pixels in the image, its computation is highly scalable with respect to image resolution. As a matter of fact, it is always carried out over the fixed number of 256 gray levels. Moreover, being region-based rather than pixel-based, the measure is also more robust to slight differences in orientation.
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https://doi.org/10.1007/BFb0077993combine the two vectors, the classification results are better than the one obtained using only one set of features. The classification was performed on the Brodatz album, using a naive Bayes classifier.
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https://doi.org/10.1007/BFb0058488ctor. For the identification a nearest neighbor classification is used. The evaluation is performed on the ., ., and the . datasets. Experiments show, that this novel approach achieves better results to previously presented writer identification approaches.
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,Un théorème d’image directe propre,ts, mutual information and Census transform. We also compare two different disparity estimation methods, graph cuts and semi-global matching. The results show that the overall quality of the fused images is near the reference images.
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