Fig. 32
Residuals from a global G − GRP = f(GBP − GRP) relation for asample of luminous, low extinction stars (A0 < 0.05 mag, MG < 4 mag). Top: as a function of G, colour-coded by the number of stars normalised by the total number of stars per magnitude bin. Bottom: as a function of GBP − GRP for a sample of bluer stars, colour-coded by the magnitude.
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