Fig. 6

Atmospheric models fitted to the observed spectra and photometry of HD 206893 B shown in the background. Dark red lines show the best fit dusty models that include additional extinction by high-altitude dust clouds made of enstatite grains and light red lines show the exact same models before applying the extinction (i.e., without dust). The GPI spectra are not to be taken to face value since they are rescaled during each of the fits. BT = BT-Settl-CIFIST, DP = DRIFT-PHOENIX, and ER = Exo-REM.
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.