Free Access
Fig. 14

Planet mass detection limits (5σ) for the IRDIS K1-band and NaCo L′-band images, both with the effect of attenuation of a planet emitted flux by protoplanetary dust (dashed and dash-dotted curves, see text) compared to the case where the attenuation by protoplanetary dust is neglected (solid curves, see Fig. 12).
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.