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Fig. 8.
Ratio of the thick- and thin-disc masses (i.e., ΣT/Σt) of the PSF-deconvolved model fits as a function of the circular velocity (vc) for the galaxies in our sample with circular velocity information (see Table 2). Overplotted are the values of the sample in Comerón et al. (2018), labeled as C18.
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