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Fig. 40
GaiaG vs. GBP and GRP photometry. Residuals of G-GRP from a global G-GRP=f(GBP−GRP) spline as a function of G magnitude. The red line is a smoothed spline fit. The sample contains 10 000 stars with a uniform distribution in magnitude; therefore, the lighter grey scale indicates less dispersion in the residuals.
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