Emitted light spectral energy distribution λLp,em,λ (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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.