Fig. 3.
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Comparison between the SMF of the COSMOS2020 sample (Weaver et al. 2023, 2022) and the SMF of the sources studied in this paper. The SMF was obtained by counting the galaxies in each redshift bin separately for each cluster and dividing by the corresponding volume, corrected for the mean magnification of the sources in each bin. The error bars correspond to the 16th to 84th percentile of the stellar mass of the sources in the sample, and the impact of the 20% error on the magnification on the total volume.
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