Fig. 4.
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Our Υd (circles) and Υb (triangles) values as a function of disc luminosity (Ld). We distinguish between galaxies with photometry at 1.65 μm and 3.6 μm. The lines and bands represent the Gaussian priors adopted for Υd in our mass modelling (see Sect. 4 and Appendix C). The prior for Υb was flat within Υd < Υb < 2 Υd (not shown).
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