Fig. 3.
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Same as for Fig. 2, but we report only the relation by V15 (solid brown line) and we separate the LFs by the different galaxy populations (coloured lines): spirals (dotted light green), SBs (loosely dashed cyan), SF-AGN (dashed dark green), SB-AGN (densily dashed orange), AGN1 (loosely dash-dotted blue), AGN2 (dash-dotted magenta), and dwarf irregulars (dash-dot-dotted brown).
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