Fig. 2

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PSD of high-pass filtered (Rc = 100) planet spectrum (T = 500 K, log(g) = 4, [M/H] = 0) for two different resolutions on the total spectral range offered by BT-Settl spectra (0.3–12 µm). The hatched areas correspond to the areas under the curves equal to the quantity α2. Note: the PSD has been smoothed only for better visualization purposes. The y-axis is relative to the total flux of the companions. Only the ratios between the curves explaining the a variation from a given resolution to another one should be taken into consideration.
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