Fig. A.1.
Extinction laws for the CoRoT band (in black) and for the V, Rc, and Ic optical filters (green, red, and orange, respectively). The thin lines show the variation of A(band)/AV with effective temperature for the stellar-like spectra with log g between 3.0 and 4.5. Thicker lines show the trend of A(band)/AV with temperature for black body spectra.
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