Euclid preparation - XLIII. Measuring detailed galaxy morphologies for Euclid with machine learning

Open Access

Fig. 3

Vote fraction mean deviation averaged over all morphology answers $\bar{δ}$ $\[\bar{\delta}\]$ as a function of the number of galaxies N_train from the bright and complete set used for training. To ensure a consistent comparison, the predictions were done on the complete test set. Lower values indicate better performance.

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