Fig. C.1.
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Relations between disc luminosity and disc mass-to-light ratio exploited to set our mass models priors. Data (from Marasco et al. 2025) are shown with red (3.6 μm) and green (1.65 μm) markers. Our best-fitting exponential functions and the adopted uncertainties are shown with colour lines and bands. These exponential fits are imposed as priors during our mass models in Sec. 4.
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