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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.

This figure is made of several images, please see below:

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