Free Access

Fig. 3.

image

Download original image

Recovered FVG host-galaxy fluxes (gal) for various S/N and time sampling. The distributions obtained for the CS are shown with the same colors as the light curves in Fig. 2. To facilitate comparison, we show in black the distributions obtained for the HS. The FVG applied to the CS appears to be considerably better than the HS; it is characterized by the smallest dispersion around the true galaxy (gal0; vertical dotted black line) for an S/N > 100 (see text).

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.