Fig. B.3

Luminosity-weighted and mass-weighted stellar age (upper and lower map, respectively) in Gyr (right-hand vertical bar) determined from Starlight fits to individual spaxels. A trend for decreasing age with radius is apparent, in qualitative agreement with the results by González Delgado et al. (2014a). The ⟨ t⋆ ⟩ ℳ map indicates a mass-weighted stellar age of ≥7 Gyr throughout the optical extent of the ETG.
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