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Fig. 8
Left: observed continuum flux at 1275 Å vs. the flux at 5100 Å for NGC 4151 obtained during short-time period (see text for details). Right: modeled continuum flux at 1275 Å vs. the flux at 5100 Å (solid lines for different RBLR sizes, denoted in the bottom left) compared to the observed values (full circles).
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