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Fig. 9.
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Comparison of the bar fraction distribution with stellar mass of the SMACS0723 cluster (violet) and in the field at z = 0 (Méndez-Abreu et al. 2012), i.e., low-density environments (green). The arrow at (log(M⋆/M⊙)∼9.3) marks the minimum thickness of discs for galaxies in the field (see Sánchez-Janssen et al. 2010).
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