Fig. C.1
Comparison between stellar mass estimates and the ratio between the NASA Sloan Atlas estimation (top), the (Chang et al. 2015) estimation (middle) and the MPA-JHU estimation (bottom) with our stellar mass. The solid line shows the median value and dashed lines show the ± 1σ dispersion. Colors represent the apparent diameter of the galaxies in arcminutes. Crosses show sources classified as interacting galaxies and circles show non-interacting galaxies.
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