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Fig. 5.
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Radial profiles of recent (100 Myr) SFRs of the different source groups, discussed in Sects. 4.1 and 4.2. The lines show the median SFRs and the shaded regions mark the 25th and 75th percentile values of the SFR distributions. SFRs for the non-AGN group are larger at every radial point than the AGN groups.
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