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Fig. A.1
A TEff = 3600 K M dwarf strongly contaminated (cλ=600 nm = 0.85) by a TEff = 5800 K G star. Upper panel: relative stellar fluxes as a function of wavelength; middle panel: contamination factor as a function of wavelength; bottom panel: radius ratio factor (ktrue ∕kapp) as a function of wavelength.
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