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Fig. 13

image

Upper panel: star formation rate plotted in four bins of redshift for the complete sample of quasars. We adopt different criteria for separating strong-outflow (small magenta points) and weak-outflow galaxies (small green points), respectively higher and lower than the median value of the distribution of the three parameters (νblue (first panel), Δνoffset  (second panel), and Δνσ [O III] ). Bottom panel: same as top, but excluding radio loud quasars.

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