Examples of spectra (J092620.62+101734.8 and J113651.66+445016.4, respectively) from our sample where the host galaxy mimics strong Fe II emission, leading to a mistaken identification of strong FeII emitters. Spectra on the plots (a) and (b) have a widely different S/N. The panels show as follows (from top to bottom): the real spectra and the best fitting model; the smoothed spectra overlapped with the best fitting model; single stellar population spectra that were used in the best fitting model; and the Fe II template used in the fit. Some prominent absorption lines are marked on the plots.