Fig. 5.
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Change in the position in the BPT diagram for 101 galaxies of the matched sample from this work with the RCSED catalog. At the base of the arrow is the position determined by the emission line fluxes from the RCSED without decomposition, and at the top of the arrow is the position determined by the narrow component as a result of decomposition into narrow and broad components. The color code denotes the distance between the two measures in the diagram.
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