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Fig. A.1.

image

Distribution of the longest time delay Δtmax for the non-selected lensed quasars and the selected lensed quasars. Top panel: mean values of Δtmax with 1 standard deviation as the error bars from the lensed quasars in each θLP bin. Middle panel: number of non-selected lensed quasars, the number of selected lensed quasars, and the number of total mock lenses in each θLP bin. Bottom panel: TPR in each θLP bin. The sensitivity of the lens search algorithm mainly comes from the separation (θLP), not the time delay (Δtmax).

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