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Difference between output from fado for spectral fits with the Base ℱ and input value of stellar mass ℳ⋆a), mean light- and mass-weighted stellar age b) and c), mean light- and mass-weighted stellar metallicity d) and e), and mean percentual deviation of the Hα emission-line equivalent width f). The synthetic input spectra were computed with Rebetiko assuming an instantaneous burst star formation scenario. In panel f) the blue points correspond to equivalent-width of Hα in emission below 0.5 Å and the magenta points mark values in the range 0.5 Å ≤ EW(Hα) ≤ 1 Å. The green lines are three times the standard deviation over the whole age range of the models. The vertical blue strips on top of the diagrams depict the ages of the SSPs composing Base ℱ.
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