Fig. C.1
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Wavelength-dependent pressure level at which the optical depth due to cloud particles becomes unity, τ = 1, i.e pgas = p(τλ = 1), for a grid model planet with Upper Left: an F-type host star, Upper Right: a G-type host star, Lower Left: a K-type host star, and Lower Right: an M-type host star, each at Teff,p = 800, 1600 and 2400 K, log(g) = 3 [cgs]
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