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Fig. A.1

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Residuals between BP-RP colors and fitted polynomials as a function of effective temperature (left), metallicity (middle), and the histogram of these residuals. The top row shows the result for stars with [Fe/H]>-0.25, and the middle row for stars with −0.75<[Fe/H]<-0.25 and [Fe/H]<-0.75.

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