Fig. 6
Correlation of the EW Hβ with the incident luminosity of the continuum at 5100 Å for different RBLR (denoted in the bottom left), obtained from the Cloudy simulations. Circles represent observed intrinsic Beff for the Hβ line of NGC 4151 with continuum fluxes corrected for the host-galaxy contribution (zoomed-in for better visibility).
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