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Fig. F.1.


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Percentage variation of the apparent radius R estimated neglecting the presence both of absorption and reddening, with respect to the true radius R0 of a solar-type star (with effective temperature Teff = 5772 K) as a function of reddening E(GBP − GRP) (solid line). The dashed and dotted lines represent the apparent radius variation resulting from neglecting either the reddening (dashed) or the absorption (dotted), respectively.

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