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Fig. 4


Stacked distribution of F160W magnitudes of galaxy members in the core of MACS 0416. Spectroscopically confirmed members from CLASH-VLT (Balestra et al. 2016) are shown in blue (80), the newly identified members by MUSE in green (73) and the remaining photometrically selected galaxies with magF160W < 24 from Gr15 in red (193 in total). The stellar mass on the top axis is computed from log (M/M) = 18.541−0.416 × magF160W from Gr15.

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