Fig. 5.
Top panel: Gaussian decomposition and iron fit for galaxy 2MASX J01464481−0040426. The observed spectrum flux is in arbitrary units (thick line); FeII template and Gaussian components obtained with LINER are in thin lines. The residual spectra are plotted on the lower sub-panel for clarity. Bottom panel: zoomed in view of the Hβ + [OIII] observed spectrum and its fit.
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