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Fig. 10
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Distribution of estimated stellar mass differences compared to GSWLC (ΔMGSWLC; Salim et al. 2016, 2018, upper panel) and LoTSS Deep Fields DR1 (ΔMDF; Duncan 2022, lower panel) for sources in common. Red circles and corresponding error bars illustrate the median and 16-84th percentile ΔM within a fixed log10(MLoTSS/M⊙) bin.
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