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Fig. 5.


Fitted and calculated color gradients of each individual early-type galaxy plotted against the respective cluster-centric distance (left), integrated magnitude in I814 (middle) and stellar mass (right). The same color scheme as in Fig. 4 applies. The dashed, gray line indicates a null color gradient. Based on Pearson correlation coefficients we detect no dependence between color gradients and those galactic properties, independent of color and method.

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