Fig. 6
Difference between the MB posterior derived from BPZ2 and the B-absolute magnitude provided by MUFFIT for a common sample of I ≤ 23 ALHAMBRA galaxies at 0.2 ≤ z< 1.0 (black histogram). The red solid curve shows the best Gaussian fit to the distribution, with median μ = 0.05 mag and dispersion σ = 0.18 mag. The dashed line marks identity.
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