In the three tables below, the 436 candidate systems from Dawes et al. 2022 (submitted) are grouped by Grade, each Grade is arranged by ascending RA. For each image, N is up, and E to the left. The columns are arranged as follows:

[0] Index for each unique system; [1] Cutout image (2-4 images per system); [2] Name of the system (RA and Dec in decimal format); [3] Human inspection grade; [4] Spectroscopic redshift of quasars from SDSS DR16 and/or SNIFS (with an asterisk); [5] Photometric redshift of putative lensing galaxies; [6] g band magnitude; [7] r band magnitude; [8] z band magnitude; [9] Parallax significance; [10] Proper motion significance; [11] Double or quad; [12] Average separation of images

The tables below are google sheet and are available for download in csv (ascii) format here.