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Table B.1.

Comparison of true-positive (TP) and false-positive (FP) rates for different selection criteria using the photometric redshift distributions around the 546 grade A or B lens candidates.

No. Criteria visual insp. Literature F1 statistics
Nmax zlow zlow Ntot Nfrac Npeak5 Apeak5 Npeak10 Apeak10 TP FP TP FP F1vis F1lit F1tot
0 ≥0 ≥0 ≤inf ≥0 ≥0 ≥0 ≥0 ≥0 ≥0 84 462 174 372 0.210 0.483 0.358
1 ≥15 ≥0.1 ≤1.0 ≥400 ≥0.025 ≥0 ≥0 ≥0 ≥0 68 188 119 137 0.425 0.553 0.499
2 ≥15 ≥0.1 ≤1.0 ≥400 ≥0.026 ≥0 ≥0 ≥0 ≥0 67 167 115 119 0.450 0.564 0.516
3 ≥15 ≥0.1 ≤1.0 ≥400 ≥0.027 ≥0 ≥0 ≥0 ≥0 64 146 109 101 0.467 0.568 0.526
4 ≥15 ≥0.1 ≤1.0 ≥500 ≥0.025 ≥0 ≥0 ≥0 ≥0 65 170 111 124 0.435 0.543 0.497
5 ≥15 ≥0.1 ≤1.0 ≥500 ≥0.026 ≥0 ≥0 ≥0 ≥0 64 149 107 106 0.462 0.553 0.515
6 ≥15 ≥0.1 ≤1.0 ≥500 ≥0.027 ≥0 ≥0 ≥0 ≥0 61 128 101 88 0.482 0.556 0.526
7 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥0 ≥0 ≥0 ≥0 68 161 113 116 0.464 0.561 0.520
8 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.026 ≥0 ≥0 ≥0 ≥0 67 144 109 102 0.487 0.566 0.533
9 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥0 ≥0 ≥0 ≥0 64 124 103 85 0.508 0.569 0.544
10 ≥15 ≥0.1 ≤0.8 ≥500 ≥0.025 ≥0 ≥0 ≥0 ≥0 65 144 106 103 0.476 0.554 0.521
11 ≥15 ≥0.1 ≤0.8 ≥500 ≥0.026 ≥0 ≥0 ≥0 ≥0 64 127 102 89 0.502 0.559 0.535
12 ≥15 ≥0.1 ≤0.8 ≥500 ≥0.027 ≥0 ≥0 ≥0 ≥0 61 107 96 72 0.526 0.561 0.547
13 ≥17 ≥0.1 ≤1.0 ≥400 ≥0.025 ≥0 ≥0 ≥0 ≥0 63 139 106 96 0.474 0.564 0.526
14 ≥17 ≥0.1 ≤1.0 ≥400 ≥0.026 ≥0 ≥0 ≥0 ≥0 62 128 105 85 0.488 0.577 0.540
15 ≥17 ≥0.1 ≤1.0 ≥400 ≥0.027 ≥0 ≥0 ≥0 ≥0 60 114 100 74 0.504 0.575 0.546
16 ≥17 ≥0.1 ≤1.0 ≥500 ≥0.025 ≥0 ≥0 ≥0 ≥0 61 130 102 89 0.478 0.559 0.526
17 ≥17 ≥0.1 ≤1.0 ≥500 ≥0.026 ≥0 ≥0 ≥0 ≥0 60 119 101 78 0.494 0.572 0.540
18 ≥17 ≥0.1 ≤1.0 ≥500 ≥0.027 ≥0 ≥0 ≥0 ≥0 58 105 96 67 0.511 0.570 0.546
19 ≥17 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥0 ≥0 ≥0 ≥0 63 120 101 82 0.510 0.566 0.543
20 ≥17 ≥0.1 ≤0.8 ≥400 ≥0.026 ≥0 ≥0 ≥0 ≥0 62 112 100 74 0.521 0.575 0.553
21 ≥17 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥0 ≥0 ≥0 ≥0 60 98 95 63 0.541 0.572 0.560
22 ≥17 ≥0.1 ≤0.8 ≥500 ≥0.025 ≥0 ≥0 ≥0 ≥0 61 111 97 75 0.517 0.561 0.543
23 ≥17 ≥0.1 ≤0.8 ≥500 ≥0.026 ≥0 ≥0 ≥0 ≥0 60 103 96 67 0.529 0.570 0.553
24 ≥17 ≥0.1 ≤0.8 ≥500 ≥0.027 ≥0 ≥0 ≥0 ≥0 58 89 91 56 0.550 0.567 0.560
25 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥7 ≥50 ≥1 ≥15 67 149 110 106 0.479 0.564 0.528
26 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥7 ≥70 ≥1 ≥15 66 145 109 101 0.480 0.568 0.531
27 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥1 ≥15 ≥2 ≥26 66 128 106 88 0.512 0.576 0.550
28 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥1 ≥15 ≥2 ≥30 66 117 100 82 0.534 0.562 0.551
29 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥7 ≥50 ≥1 ≥15 63 114 101 76 0.523 0.575 0.554
30 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥7 ≥70 ≥1 ≥15 62 95 100 73 0.561 0.576 0.570
31 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥1 ≥15 ≥2 ≥26 62 100 97 65 0.549 0.577 0.566
32 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥1 ≥15 ≥2 ≥30 61 91 92 60 0.565 0.564 0.565
33 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥10 ≥50 ≥1 ≥15 65 122 99 88 0.518 0.548 0.536
34 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥10 ≥70 ≥1 ≥15 65 122 99 88 0.518 0.548 0.536
35 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥7 ≥50 ≥1 ≥26 65 121 103 83 0.520 0.572 0.551
36 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.025 ≥7 ≥70 ≥1 ≥26 64 119 102 81 0.518 0.571 0.550
37 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥10 ≥50 ≥1 ≥15 61 96 93 64 0.552 0.562 0.558
38 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥10 ≥70 ≥1 ≥15 61 79 93 64 0.598 0.562 0.576
39 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥7 ≥50 ≥1 ≥26 61 95 95 61 0.555 0.576 0.567
40 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥7 ≥70 ≥1 ≥26 60 95 94 60 0.548 0.573 0.563
41 ≥15 ≥0.1 ≤0.8 ≥470 ≥0.027 ≥10 ≥50 ≥1 ≥15 61 92 91 62 0.562 0.557 0.559
42 ≥15 ≥0.1 ≤0.8 ≥470 ≥0.027 ≥10 ≥70 ≥1 ≥15 61 76 91 62 0.607 0.557 0.576
43 ≥15 ≥0.1 ≤0.8 ≥470 ≥0.027 ≥7 ≥50 ≥1 ≥26 60 91 92 59 0.558 0.566 0.563
44 ≥15 ≥0.1 ≤0.8 ≥470 ≥0.027 ≥7 ≥70 ≥1 ≥26 59 91 91 58 0.551 0.563 0.559
45 ≥15 ≥ 0.1 ≤0.8 ≥470 ≥0.027 ≥10 ≥100 ≥1 ≥15 61 75 91 58 0.610 0.563 0.580
46 ≥15 ≥0.1 ≤0.8 ≥470 ≥0.027 ≥10 ≥120 ≥1 ≥15 58 67 87 49 0.614 0.561 0.581
47 ≥15 ≥0.1 ≤0.8 ≥470 ≥0.027 ≥7 ≥100 ≥1 ≥26 59 77 86 50 0.590 0.555 0.569
48 ≥15 ≥0.1 ≤0.8 ≥470 ≥0.027 ≥7 ≥120 ≥1 ≥26 57 67 82 42 0.606 0.550 0.572
49 ≥15 ≥0.1 ≤0.8 ≥400 ≥0.027 ≥5 ≥50 ≥2 ≥26 62 98 96 64 0.554 0.575 0.566
50 ≥15 ≥0.1 ≤0 ≥0 ≥0 ≥0 ≥0 ≥0 ≥0 76 284 147 213 0.358 0.551 0.466
51 ≥0 ≥0.1 ≤0 ≥470 ≥0 ≥0 ≥0 ≥0 ≥0 79 364 151 292 0.312 0.489 0.409
52 ≥0 ≥0.1 ≤0 ≥0 ≥0.027 ≥0 ≥0 ≥0 ≥0 70 227 127 372 0.388 0.377 0.381
53 ≥0 ≥0.1 ≤0 ≥0 ≥0 ≥10 ≥0 ≥0 ≥0 75 267 133 209 0.369 0.516 0.451
54 ≥0 ≥0.1 ≤0 ≥0 ≥0 ≥0 ≥120 ≥0 ≥0 67 199 130 186 0.406 0.531 0.480

Notes. We distinguish between lens candidates classified as clusters during visual inspection (see Sect. 4.2) and based on galaxy catalogs (Oguri 2014; Oguri et al. 2018; Wen & Han 2018, 2021). Without photo-z selection (see No. 0), we visually identified 84 lens candidates to be in an overdense environment, while 174 lens candidates are located closer than 100″ from a known galaxy cluster. We highlight No. 46 in bold, which has the selection criteria cuts that are the best according to the F1tot statistic.

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