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Fig. 4.

image

ΔBC = BCAV − BCAV = 0 as a function of Teff for Gaia G band (left panel), Gaia GBP − GRP colour (central panel), and the WFC3/UVIS F218W filter (right panel). The grey open circles denote the models with fixed extinction coefficients at the filter centres, which are connected by the solid lines. The dashed lines indicate a linear extrapolation of the open circles of AV = 0 and AV = 1 mag, for the same Teff. The ATLAS9 models are used in this figure, but the PHOENIX models give consistent results.

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