Fig. 12.

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Strongly lensed L1 (left panel) and L2 (right panel) detection rates per effective year of observation for u, g, r and i bands assuming a variable peak magnitude, mlim, peak. The mlim, peak ranges for ZTF and LSST1 assuming a survey area of 20 000 deg2 are shown in gray and pink, respectively. The LSST1 mlim, peak values for each of the four bands are overlaid along the curves in stars, and the ZTF mlim, peak values for g, r and i are overlaid along the curves in diamonds.
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