Fig. B.1
Left panel: magnitude error as a function of odds and pdz_best parameter for MACS1206 galaxy cluster. The black dots and blue stars show respectively Le Phare and BPZ results. Right panel: percentage of galaxies left after a cut in the pdz_best parameter for Le Phare in solid lines and odds parameter for BPZ in dashed lines for MACS1206 galaxy cluster at different F814W magnitudes limit.
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