Free Access

Fig. 1

image

Distribution of galaxies in SALL sample in the Log SFR – Log M plane. Top panels: SFR distribution of galaxies in three different stellar mass bins. The red solid line is the result of the gaussian fit to the right-side of the SF peak. Bottom panel: Log SFR – Log M plane colour-coded as a function of the number of galaxies in each bin. The contours encircle bins that host a number of galaxies from 50 to 1250, with step of 250. The MS of SFGs is indicated by the thick solid line, while the error bars mark the 1σ scatter.

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.