Evidence of a diffuse, extended continuum source in quasars from the relative sizes of the broad line region and the UV-optical continuum source measured with microlensing

Open Access

Fig. 1.

Posterior probability densities of the ratio of the BLR inner radius, r_in BLR, over the continuum source outer radius, r_s Cont. The object – line (– date) combinations are indicated in the left corners. In the right corners, we give the median values of the probability distributions and their uncertainties (see text). The dotted line indicates where r_in BLR = r_s Cont.

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