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Fig. 7.

image

λReϵ relation as a function of location in the star-formation rate versus total stellar mass (M) relation for the CALIFA galaxies. Each panel shows the complete sample highlighting in color the ones belonging to each specific SFR–M bin. The number in each subpanel gives the -weighted λRe average for the highlighted galaxies in that bin. The dark gray dashed line in the SFR versus M on the right marks the division between the main star-forming sequence and quiescent galaxies from Renzini & Peng (2015).

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