Table 1.
Subsample of CLASH clusters.
| Cluster | Redshift | Nsrc | Nimage | Nbk |
|---|---|---|---|---|
| Abell S1063(2) | 0.351 | 20 | 55 | 41 |
| MACS J0329.7–0211(1) | 0.450 | 9 | 23 | 19 |
| MACS J0416.1–2403(3) | 0.397 | 66 | 182 | 59 |
| MACS J0429.6–0253(1) | 0.399 | 3 | 11 | 41 |
| MACS J1115.9+0129(1) | 0.352 | 3 | 9 | 30 |
| MACS J1206.2–0847(2) | 0.441 | 27 | 82 | 23 |
| MACS J1311.0–0310(1) | 0.494 | 3 | 8 | 17 |
| MACS J1931.8–2635(1) | 0.352 | 7 | 19 | 16 |
| MACS J2129.4–0741(1) | 0.587 | 11 | 38 | 40 |
| RX J1347.5–1145(1) | 0.451 | 8 | 20 | 18 |
| RX J2129.7+0005(1) | 0.234 | 7 | 22 | 76 |
Notes. The lensing analysis, cluster redshifts, and the number of identified counterparts of the lensed sources are from Caminha et al. (2019) (1), Bergamini et al. (2019) (2), and Vanzella et al. (2021) (3). Nsrc is the number of unique sources (single galaxies or resolved clumps within a galaxy) that are multiply lensed, and Nimage is the total number of images of the lensed sources identified in each field. In the last column we list the number of additional background sources in the FOV that do not have multiple counterparts.
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