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Fig. C.2
Radial profile of M/L5635 derived from the ratio between μ⋆ and L5635 (the luminosity measured at the normalized wavelength corrected by the stellar extinction) obtained for GM (black) and CB (grey) bases. M/L at the observed 1.6 μm and at the synthetic 1.6 μm are shown as dashed-red and solid-red lines, respectively.
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