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Fig. 25

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Comparison between TOPz and GAMA stellar masses for each galaxy. The x-axis shows the GAMA stellar masses acquired using GKV ProFound photometry (see Sect. 3). The y-axis shows the TOPz stellar masses that are computed using the spectral templates from the CIGALE software (see Sect. 2.5). The colour denotes the TOPz photo-z accuracy. The dashed black line is a median stellar mass ratio relation, where M★,TOPz ≈ 1.3 ⋅ M★,GAMA. Galaxies where TOPz photo-z are close to the spectroscopic redshiſts follow the stellar masses from the GAMA database very well.

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