Fig. 13.

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Distributions of the lensing properties of the strongly lensed L2 systems from detections in each of the u, g, r and i bands after applying image separation cuts and LSST1 magnitude cuts. Top panels from left to right: lens galaxy redshift zl, TDE redshift zs, and image separation θsep. Bottom panels from left to right: lensed magnitude (magnitude of the fainter image in a double system or the third brightest image in a quadruple system), stellar velocity dispersion σ of the lens galaxy, and time delays tdelay of all images in the lensed systems.
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