Fig. 16

Relative position and contrast of GJ 676A b in the WFIRST blue channel projected onto the sky plane for an albedo of 0.5. In combination with Fig. 15, this allows for optimal planning of direct-imaging observations. The data is the same as the one underlying Fig. 15. Contrast contours are shown for the ensemble of orbital solutions and the solid line shows the best-fit solution. Dashed and dotted circles indicate separations of 50 mas and 100 mas, respectively, from the host star marked with a cross.
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.