Free Access
Fig. 6
Speckle noise estimation for HR8799b observed on December 6, 2014. The histograms illustrate the offsets between the true position/flux of a fake companion and its position/flux obtained from the NEGFC technique. The dashed lines correspond to the 1D Gaussian fit from which we determine the speckle noise.
This figure is made of several images, please see below:
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.