Fig. C.1.
Download original image
Correction of the absolute continuum level in the extreme blue of a cool star. Top: comparison between the GJ576 master spectrum coming out from RASSINE (black curve) and the best-fitted template model (red curve). The star is an M1.5 dwarf for which the best stellar template in ATLAS is a model with T = 4100 K and log(g) = 5.0. We show, in orange, the correction curve for the continuum absorption. Bottom: RASSINE master spectrum after template correction. The accuracy in the blue is considerably improved.
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.