Fig. A.1.

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Resulting posterior distributions on all the free parameters for our cosmological model using the three different configurations: fiducial model (in grey), stellar masses corrected using the best approximation with LEPHARE-NL (in orange), and stellar masses corrected with the average difference among different codes (in green). The contour levels correspond, from inside out, to 68%, 95%, and 99% of the posterior distribution.
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