Abstract
Galaxies morphology classification is a crucial task for studying their physical properties, formation and evolutionary histories. The large-scale surveys on universe has boosted the need to develop techniques for automated galaxies morphological classification. This paper proposes a system able to classify automatically galaxies according to the Hubble De Vaucouleurs diagram. We introduce a novel CNN architectures that for the first time was trained to automatically classify galaxies according to 26-classes Hubble-De Vaucouleurs scheme. We use Galaxy Zoo dataset, using the decision tree, to extract a labeled examples containing an even amount of images of each 26-classes. We also compared different CNN Backbones in order to assess obtained galaxies classification results. We obtain a balanced multi-class accuracy (BCA) of more than 80% in classifying all 26 Hubble-De Vaucouleurs galaxy categories.
The authors thank Arturo Argentieri for his technical support in the setup of the hardware used for network training and data processing.
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Mazzeo, P.L., Rizzo, A., Distante, C. (2022). Morphological Galaxies Classification According to Hubble-de Vaucouleurs Diagram Using CNNs. In: Sclaroff, S., Distante, C., Leo, M., Farinella, G.M., Tombari, F. (eds) Image Analysis and Processing – ICIAP 2022. ICIAP 2022. Lecture Notes in Computer Science, vol 13231. Springer, Cham. https://doi.org/10.1007/978-3-031-06427-2_5
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