Fig. 3
GALFIT input and output for three galaxies of the magnitude limited sample. In the upper panels are the images of the galaxies in the F850LP filter, in the middle panels the best fitting Sérsic model profiles, and in the lower panels the residual images obtaining by subtracting the model from the image. The first two columns illustrate examples of late morphology galaxies with a best fitting Sérsic index n> 2.5, while the last column displays an elliptical galaxy with n < 2.5.
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.