Fig. 7.
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Confusion matrix of morphological bar classes from this work compared to literature classes from Buta et al. (2015) for S4G using IRAC 3.6 μm images and de Vaucouleurs et al. (1991) otherwise (=RC3), based on optical and infrared images. The values of each column sum up to 100%. We note that none of our galaxies has a literature bar class of S
B, thus no column is added.
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