Fig. 1.
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AGN monochromatic luminosity at 5100 Å as a function of the BH mass. The error bar in the bottom right corner represents the typical uncertainty of the quantities. The dashed lines correspond to fixed Eddington ratios. The contours show the distribution of the broad-lined AGNs taken from the 7th data release of the Sloan Digital Sky Survey (SDSS; Abolfathi et al. 2018) at z < 0.35 presented by Liu et al. (2019).
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