Fig. 11.
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Relation between the radius of the C IV BLR, that is, the rest-frame time lag from reverberation mapping and the continuum luminosity at 1350 Å, with different fits superimposed as continuous lines (from Kaspi et al. 2021). The BLR half-light radii measured from our microlensing analysis of the quasars J1004+4112 and Q2237+0305 are superimposed in red.
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