Free Access

Fig. 4.

image

Comparison of radial profiles of Σ: the original profile estimated from the stellar population results (continuous line), the profile derived from our MLCRs calibrated using all galaxies (dashed line), and the MLCRs by Hubble type (dotted line), for NGC 6063 and NGC 2880 (same galaxies as in Fig. 1). The Σ profiles derived from the MLCRs have been obtained from the g − r 2D color map and the Lg 2D map. For the sake of clarity, only the uncertainty band from the Hubble type MLCR has been plotted (the others are on the same order).

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.