Fig. 7.
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Example of SED modelling results for two extreme gradient values: A2GS26 (orange) with a SFR gradient over 100 Myr of −48° and A2GS50 (blue) with a gradient of 60° over the same period. Circles are flux densities, while solid lines are the best fits. The SEDs are normalised to their rest-frame 2 μm flux densities, which is a proxy for stellar mass.
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