Table 1.
Description of the cluster sample included in the GGSL simulation.
| Cluster | zcluster | Survey | M200c(a) [1014 M⊙] | Nimg | NCLM ( ) |
Δrms [″] | Ref. | |
|---|---|---|---|---|---|---|---|---|
| RX J2129+0005 | R2129 | 0.234 | CLASH | 7.8±2.4 | 22 | 70 (34) | 0.20 | (1) |
| RX J2248–4431 (b) | R2248 | 0.346 | HFF | 19.8±6.0 | 55 | 222 (115) | 0.55 | (2) |
| MACS J1931–2635 | M1931 | 0.352 | CLASH | 11.6±8.8 | 19 | 120 (59) | 0.38 | (1) |
| MACS J0416–2403 | M0416 | 0.397 | HFF | 11.4±2.7 | 182 | 193 (49) | 0.40 | (3) |
| MACS J1206–0847 | M1206 | 0.439 | CLASH | 15.1±3.2 | 82 | 258 (147) | 0.46 | (2) |
| MACS J0329–0211 | M0329 | 0.450 | CLASH | 12.7±2.2 | 23 | 106 (49) | 0.24 | (1) |
| RX J1347–1145 | R1347 | 0.451 | CLASH | 35.4±5.1 | 20 | 114 (70) | 0.36 | (1) |
| MACS J2129–0741 | M2129 | 0.587 | CLASH | 1.84±0.01 (c) | 38 | 138 (45) | 0.56 | (1) |
Notes. The first three columns list the: cluster names, short names, and redshifts. The fourth column specifies the program from which the images are extracted. Nimg (Col. 5) is the number of multiple images used to constrain the model, NCLM (Col. 6) is the number of CLMs used to describe the subhalo mass component (the number of CLMs photometrically selected is given in parentheses), Δrms (Col. 7) is the root-mean-square separation between the observed and model-predicted multiple image positions. The reference lens model for each cluster is quoted in the last column.
The cluster virial mass values were measured through weak lensing by Umetsu et al. (2018).
The weak lensing measurement is not available for M2129; we report here the mass within 200 kpc from Caminha et al. (2019).
References. (1) Caminha et al. (2019); (2) Bergamini et al. (2019); (3) Bergamini et al. (2021a).
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