Fig. 17


Top panel: normalised mean bias in photometric redshift estimates as a function of apparent magnitude of the galaxy. Bottom panel: same, but now against the F775WF160W colour. The dashed black lines show the level corresponding to a bias of ± 10-2. The blue dashed line shows the trend found when considering galaxies with secure (confidence ≥ 2) MUSE redshifts.

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