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

Open Access

Fig. 15

Redshift and magnitude dependence of the ‘has-spiral-arms’ vote fraction mean deviations δ_i for the model trained on the original HST COSMOS images. Compared to the Euclid images (Figs. 12 and 13), the deviations for high-redshift and faint galaxies are substantially smaller.

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