Fig. 2.
Graphical output of FADO. Upper panel: integrated spectrum of the M1931 BCG orange, as recovered from MUSE. The best-fitting synthetic SED is shown in light-blue, composed of the stellar and nebular continuum emission (dark green and red, respectively). Lower panel: fits to the strongest emission lines, namely, [O II] λ3727, λ3729, Hβ, [O III] λ4959, 5007, Hα, [N II] λ6584, and [S II] λ6718, 6732.
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