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Fig. 1

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Spectra (Fλ) of model atmospheres of giant planets for different effective temperatures (colored solid lines, BT-Settl models from Allard et al. 2012). Each spectrum is normalized to its value at 1.6 μm and is vertically shifted by a constant. The transmission of the three SDI filters of NaCo (T1, T2, and T3) are shown in black lines with different styles. Theoretical absorption bands of water and methane are also indicated. The vertical scale is linear.

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