Fig. B.1.
Download original image
Kinematic maps for the SAMI galaxy 9403800123. From left to right the columns show the flux, velocity, velocity dispersions and h3 and h4 Gauss-Hermite moments. From top to bottom the rows show the original data, the DYNAMITE model with correct mirroring, the DYNAMITE model with incorrect mirroring, the residuals between data and the correct DYNAMITE model divided by the kinematic uncertainties, and the relative difference between the models with correct and incorrect mirroring divided by the kinematic uncertainties.
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.