Free Access

Fig. B.8


Same as Fig. B.6, but now referring to the low-kurtosis subsample of α.btfr galaxies. The thick dashed line is the no-scatter fit to the subsample, and is the same as the thick dashed line in Fig. 6. The intrinsic scatter bands correspond to the best fit value of the parameter for the subsample, σ⊥ ,intr = 0.041 dex.

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.