Fig. 4.
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Mass outflow rates (Ṁ) as a function of AGN bolometric luminosity (adapted from Fig. 9 of Carniani et al. 2015, with permission). Teal stars represent our combined S IV sample seen in absorption. Open and filled circles indicate the Ṁ for ionized outflows determined from [O III] and H β emission lines, respectively. Squares denote molecular outflows.
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