Fig. 8
Example of the [O iii]/Hβ emission-line ratio distribution for SDSS J0233-0743. The line ratio is shown as a function of [O iii] surface brightness, distance from the QSO, and its 2D distribution before (black points) and after performing the QSO-host galaxy deblending (red points). Similar figures for all QSOs are moved to the Appendix.
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