Fig. B.1.
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Left panel: Distribution of Eddington ratios for the two quasar samples in this study, as compared to Ganguly et al. (2007). The green curves represent quasars within 1.88 < z < 2.44 with reliable Mg II-based Eddington ratios across three S/N thresholds, while the Ganguly et al. (2007) sample appears in blue. The inset shows a broader quasar sample with 1.5 < z < 4.5 and all available Eddington ratios, with the shaded region indicating the Ganguly et al. (2007) Eddington ratio distribution. Right panel: BAL fraction as a function of Log Eddington ratio for the S/N > 3 threshold sample with just ZWARNING == 0 selection filter.
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