Fig. 9.

Sensitivity to the quasar image separation θLP of the lens search method using both spatial extent and the number of blobs. Bright: the group of lensed quasars with the third brightest image brightness m3rd < 22.0 mag. Faint: the group of lensed quasars with 22.0 mag ≤ m3rd < 24.0 mag. The top panels show the TPRs of each θLP bin, when pthrs% = 0% and Nthrs = 4, with the preselection by the number of blobs Ncrit = 2. The bottom panels show the number of mock lenses in each θLP bin.
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