Fig. 2.
Distribution and mean values of the field samples according to the main parameters studied in this work: M*, Vmax, and Re. The dashed lines depict the mean values for each parameter and sample. No effective radii and rotation velocity are publicly available for the samples of Fall & Romanowsky (2018), Posti et al. (2018), and Gillman et al. (2020), while there are no stellar mass values available for Böhm & Ziegler (2016).
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