Fig. B.1
Example starlight fits for IC5376 (CALIFA 001, left), NGC 776 (CALIFA 073, middle), and UGC00312 (CALIFA 014, right). The top panels show the nuclear spectrum, while the bottom panels are for spaxels located at 1 HLR from the nucleus. Observed and synthetic spectra are shown in black and red lines, respectively. Masked regions (mostly emission lines) are plotted in magenta, and bad pixels are not plotted. Emission line peaks in the resdiual spectra were clipped for clarity.
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