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Fig. 11.

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Normalised distributions of well-classified (blue) and poorly classified (red) galaxy spectra based on various parameters (see Sect. 5 for a discussion). Top left to bottom right: Distributions as a function of redshift (z), SFR, stellar mass (Mstar), and fluxes of Hα and [OIII] emission lines. The threshold for a good prediction is set at |Δz|< 0.01.

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