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Fig. 8


Combined scattered and emitted light spectral energy distribution λLp,tot (Eq. (38)) of our HD 189733b simulation as a function of wavelength at several viewing angles α (α = 0° is the sub-stellar point). The optical wavelength scattered light luminosity drops off as the nightside of the planet is viewed. The emission features between the dayside and nightside are ~1 order of magnitude different dependent on wavelength.

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