Fig. 15
Download original image
Scaling factors for absolute flux correction, as a function of spectral type. Top panel: scaling factors applied to the UVB arm to make the spectra match the B magnitude photometry. Bottom panel: extra scaling factors applied to the VIS arm, after matching them to the R photometry, to align the UVB and VIS arms. The dotted lines in both panels correspond to ±3σ ranges.
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.