Fig. 6.
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Correlation matrix between the QSO2 outflow properties derived from the [OIII] emission line and using the flux-weighted nonparametric method, and their AGN and host galaxies properties. The Spearman rank correlation coefficients (ρ) are shown in the top right half of the matrix (blue and red), and the corresponding p-values are plotted in the bottom left half (gray).
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