Fig. C.1.
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Example of the composite stellar population modelling of the 12 OPT/NIR HST bands (left panel, open blue symbols) plus MUSE spectra (right panel, black line) of the BCG. The best fit is shown in red in both panels. In the left panel, blue empty circles and bars are the observed fluxes with 1σ errors, and filled yellow circles are model-predicted HST fluxes. In the right panel, blue areas indicate the masked regions.
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