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Fig. 12.
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B − H, V − K, and V − I color profiles of NGC 0309 at z = 0, 0.3, 0.5, 0.8, 1.5, and 2. The lower panels display the difference (in mag) relative to the true (rest-frame) color profiles of the galaxy. It can be seen that CMOD leads to a strong amplification of negative color gradients within the passively evolving bulge.
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