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Fig. 15

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Contour showing the galaxy number density as a function of the absolute magnitude in F814W and redshift for MACS1206 galaxy cluster. The absolute magnitude is derived from Le Phare photo-z fitting. The left and right panels have respectively no pdz_best cut and a cut at 0.1. The galaxy number density is in linear colour scale. The low redshift and intrisically faint galaxies show a poor photo-z estimation with pdz_best <   0.1.

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