Open Access
Fig. D.1
Download original image
Transit spectra for five different limb-darkening models. Spectra that have been fit using a re-parameterized limb-darkening law are biased towards smaller planet radii, depending on the S/N of the data. The spectra have been binned to R ≈ 50 for visual clarity.
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.