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Fig. A.1


Spectral fit with fado to a synthetic spectrum from Rebetiko corresponding to an instantaneous-burst age of 3 Myr. The input spectrum includes nebular line and continuum emission computed from the LyC photon output from the stellar component, whereby case B recombination and standard conditions for the gas were assumed. The fit was computed in the FCmode of fado with the SSP library Base . The meaning of the panels is identical to that in Fig. 3.

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