Table 1.
Summary of results for the examples.
Case | Area | Px | Mis | Good mis | Good mis | Substr. | Good px | Good px |
---|---|---|---|---|---|---|---|---|
at 10% | at 2% | mis | at 10% | at 2% | ||||
ARES | (300″)2 | 20482 | 242 | 210 | 106 | 6 | 91.7% | 67.8% |
HERA | (227″)2 | 20482 | 65 | 58 | 31 | 3 | 94.2% | 72.5% |
CL0024 | (600″)2 | 12 0002 | 19 | 17 | 13 | 0 | 99.1% | 96.1% |
CL0024 (detail) | (200″)2 | 40002 | 19 | 17 | 13 | 0 | 96.3% | 85.2% |
Notes. Name of the cluster (1st column), the area covered on the sky (2nd column), total amount of pixels (px) (3rd column), number of multiple images (mis) within the total pixel area (4th column), number of multiple images with all ratios defined in Eqs. (24) smaller than 0.1 (5th column), number of multiple images with all ratios smaller than 0.02 (6th column), number of multiple images for which at least one ratio is larger than 0.5 being a possible hint for lensing substructure (7th column), total amount of pixels with all ratios below 0.1 (8th column), total amount of pixels with all ratios below 0.02 (9th column).
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