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Fig. A.1


Comparison of several stellar population properties as obtained with the bases GMe (x-axis) and CBe (y-axis). The average difference between the property in the y- and x-axis is labeled as in each panel, and its standard deviation as σ. Panels a), b), and d) show the galaxy mass and SFR, with galaxies colored by their Hubble type. In the other panels, the values of the property measured every 0.1 HLR are compared, and the color indicates the density of points in a logarithmic scale.

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