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Fig. 2.

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Stellar mass distribution as a function of redshift of COSMOS-Web sources, with the mass completeness limits for COSMOS-Web in green (with errors calculated as the Mlim values that correspond to 85 or 95% of galaxies) and COSMOS2020 in blue as given in Weaver et al. (2022). All galaxies after magnitude filtering only are shown. Redshift bins and stellar mass thresholds, used for clustering measurements, are also represented in solid purple lines.

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