Free Access

Fig. 11


Comparison between SFRIR + UV and SFRHα when varying the dust correction for the Hα emission. The lower panel shows the case where LHα are corrected for dust attenuation by using the classical prescription of Calzetti (f = 0.58) while in the upper panel the Hα luminosities are corrected with our dust correction (f = 0.93). The black solid line is the 1:1 correlation line and the different colors indicate the stellar masses, as indicated in the vertical color bar. The lowest part of each panel also shows the median errors on the SFR measurements.

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.