Fig. 1.
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Comparison between the photometric redshifts of 43 galaxies from the final sample, for which spectroscopic redshifts are available from the literature (Liu et al. 2019). The Spearman’s rank correlation coefficient is shown as ρ, with the photometric redshift accuracy given by σMAD (Ilbert et al. 2009). The red dotted lines correspond to zp = zs ± 0.15(1 + zs) (Ilbert et al. 2009).
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