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Fig. 6


Emitted light spectral energy distribution λLp,em (Eq. (37)) of our HD 189733b simulation as a function of wavelength at several viewing angles α (α = 0° is the sub-stellar point). Spectral features remain qualitatively similar at different viewing angles with a ~1 order of magnitude difference between the sub-stellar point (α = 0°) and anti-stellar point (α = 180°). The peak wavelength is found to be at ~2 μm.

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