Table A.1.
Galaxy clusters considered in this work, with their observability conditions for HLTDS and LSST, and sources of lensing models.
| Cluster | z | RA [°] | DEC [°] | β [°] | b [°] | |β|> 54°? | LSST? | Phot. sample | source & comments |
|---|---|---|---|---|---|---|---|---|---|
| Abell 1758a | 0.280 | 203.186 | 50.543 | 53.893 | 65.297 | A, B | |||
| Abell 1763 | 0.228 | 203.834 | 41.001 | 46.323 | 73.445 | A | |||
| Abell 2163 | 0.203 | 243.954 | -6.145 | 14.899 | 30.459 | Y | C | ||
| Abell 2537 | 0.297 | 347.093 | -2.192 | 3.078 | -54.920 | Y | Y | C | |
| Abell 2813 | 0.292 | 10.853 | -20.628 | -23.162 | -83.246 | Y | A | ||
| Abell 3192 | 0.425 | 59.725 | -29.925 | -49.063 | -49.012 | Y | A | ||
| Abell 697 | 0.282 | 130.740 | 36.367 | 17.538 | 37.265 | D | |||
| ACT-CLJ0102-49151 | 0.870 | 15.734 | -49.268 | -49.963 | -67.750 | Y | Y | Caminha et al. (2023) | |
| Abell S295 | 0.300 | 41.373 | -53.041 | -63.025 | -56.570 | Y | Y | Y | D |
| CLJ0152.7-1357 | 0.833 | 28.178 | -13.955 | -23.801 | -70.561 | Y | Acebron et al. (2019) | ||
| MACS J0025.4-1222 | 0.586 | 6.388 | -12.388 | -13.890 | -74.060 | Y | A | ||
| MACS J0035.4-2015 | 0.352 | 8.859 | -20.262 | -22.037 | -82.219 | Y | A | ||
| MACS J0159.8-0849 | 0.405 | 29.955 | -8.833 | -19.703 | -65.587 | Y | Y | A | |
| MACS J0257.1-2325 | 0.505 | 44.286 | -23.435 | -38.296 | -61.418 | Y | A | ||
| MACS J0308.9+2645 | 0.356 | 47.233 | 26.761 | 8.764 | -26.781 | E | |||
| MACS J0417.5-1154 | 0.443 | 64.394 | -11.909 | -32.705 | -39.478 | Y | Y | Mahler et al. (2019) | |
| MACS J0553.4-3342 | 0.430 | 88.354 | -33.711 | -57.135 | -26.009 | Y | Y | A | |
| MS1008.1-1224 | 0.306 | 152.635 | -12.665 | -22.306 | 34.265 | Y | A | ||
| PLCK G171.9-40.7 | 0.270 | 48.237 | 8.372 | -9.204 | -40.657 | Y | E | ||
| PLCK G209.79+10.23 | 0.677 | 110.599 | 7.409 | -14.533 | 10.233 | Y | A | ||
| PLCK G287.0+32.9 | 0.390 | 177.709 | -28.082 | -26.482 | 32.907 | Y | Zitrin et al. (2017) | ||
| RXC J0018.5+1626 | 0.546 | 4.640 | 16.438 | 13.224 | -45.710 | A | |||
| RXC J0032.1+1808 | 0.396 | 8.046 | 18.133 | 13.451 | -44.499 | Y | Acebron et al. (2020) | ||
| RXC J0142.9+4438 | 0.341 | 25.730 | 44.635 | 31.448 | -17.280 | C | |||
| RXC J0232.2-4420 | 0.284 | 38.077 | -44.347 | -54.761 | -63.448 | Y | Y | A | |
| RXC J0600.1-2007 | 0.460 | 90.034 | -20.136 | -43.575 | -20.027 | Y | A | ||
| RXC J0911.1+1746 | 0.505 | 137.798 | 17.775 | 1.469 | 38.650 | A | |||
| RXC J0949.8+1707 | 0.383 | 147.466 | 17.119 | 3.763 | 47.014 | A | |||
| RXC J2211.7-0350 | 0.397 | 332.941 | -3.829 | 6.851 | -45.358 | Y | Y | C | |
| 1RXS J060313.4+421231 N | 0.228 | 90.820 | 42.245 | 18.807 | 9.737 | A, F | |||
| 1RXS J060313.4+421231 S | 0.228 | 90.851 | 42.159 | 18.721 | 9.718 | A, F | |||
| SMACS J0723.3-7327 | 0.390 | 110.828 | -73.454 | -80.187 | -23.701 | Y | Caminha et al. (2022) | ||
| SPT-CLJ0615-5746 | 0.972 | 93.966 | -57.780 | -81.031 | -27.331 | Y | Y | Paterno-Mahler et al. (2018) | |
| WHL J013719.8-082841 | 0.566 | 24.354 | -8.456 | -17.288 | -68.390 | Y | A | ||
| Abell 370 | 0.375 | 39.971 | -1.582 | -16.306 | -53.560 | Y | Y | Niemiec et al. (2023) model d1 | |
| Abell 2744 | 0.308 | 3.586 | -30.400 | -29.061 | -81.241 | Y | Y | Bergamini et al. (2023a) | |
| Abell S1063 | 0.348 | 342.183 | -44.531 | -33.825 | -59.933 | Y | Y | Beauchesne et al. (2024) | |
| 1E 0657-56 (Bullet) | 0.296 | 104.659 | -55.957 | -77.337 | -21.235 | Y | Y | G | |
| MACS J0257.6-2209 | 0.322 | 44.421 | -22.155 | -37.146 | -60.963 | Y | G | ||
| MACS J0329.6-0211 | 0.450 | 52.423 | -2.196 | -20.498 | -44.674 | Y | G | ||
| MACS J0416.1-2403 | 0.397 | 64.038 | -24.067 | -44.484 | -44.058 | Y | Y | Bergamini et al. (2023b) | |
| MACS J0451.9+0006 | 0.550 | 72.978 | 0.105 | -22.251 | -26.268 | Y | H | ||
| MACS J0520.7-1328 | 0.336 | 80.175 | -13.480 | -36.514 | -26.108 | Y | H | ||
| MACS J0940.9+0744 | 0.335 | 145.224 | 7.740 | -5.811 | 40.970 | Y | G | ||
| MACS J1206.2-0847 | 0.438 | 181.551 | -8.801 | -7.454 | 52.436 | Y | Y | G | |
| MACS J2214.9-1359 | 0.502 | 333.739 | -14.004 | -2.937 | -51.287 | Y | G | ||
| RX J1347.5-1145 | 0.451 | 206.878 | -11.753 | -0.620 | 48.808 | Y | Y | G | |
| SMACS J2031.8-4036 | 0.331 | 307.972 | -40.625 | -21.062 | -35.702 | Y | G | ||
| SMACS J2131.1-4019 | 0.442 | 322.770 | -40.322 | -24.218 | -46.921 | Y | G | ||
| SMACS J2332.4-5358 | 0.398 | 353.114 | -53.974 | -45.559 | -59.479 | Y | I | ||
| Abell 1423 | 0.213 | 179.322 | 33.611 | 30.262 | 76.659 | J | |||
| Abell 209 | 0.206 | 22.969 | -13.611 | -21.517 | -73.510 | Y | J | ||
| Abell 2261 | 0.224 | 260.613 | 32.133 | 55.117 | 31.861 | Y | J | ||
| Abell 383 | 0.187 | 42.011 | -3.533 | -18.799 | -53.502 | Y | Y | J | |
| Abell 611 | 0.288 | 120.237 | 36.057 | 15.200 | 28.900 | J | |||
| CLJ1226+3332 | 0.890 | 186.743 | 33.547 | 33.089 | 81.693 | J | |||
| MACS J0647+7015 | 0.584 | 101.959 | 70.249 | 47.054 | 25.115 | J | |||
| MACS J0717.5+3745 | 0.548 | 109.383 | 37.753 | 15.370 | 21.046 | J | |||
| MACS J0744.8+3927 | 0.686 | 116.220 | 39.458 | 17.911 | 26.652 | J | |||
| MACS J1149+2223 | 0.544 | 177.395 | 22.401 | 19.447 | 75.197 | J | |||
| MACS J1423.8+2404 | 0.545 | 215.950 | 24.078 | 35.982 | 68.985 | J | |||
| MACS J1720.2+3536 | 0.391 | 260.070 | 35.607 | 58.511 | 33.077 | Y | J | ||
| MACS J2129-0741 | 0.589 | 322.359 | -7.691 | 6.774 | -38.465 | Y | Y | J | |
| MS 2137.3-2353 | 0.313 | 325.063 | -23.661 | -9.182 | -46.937 | Y | J | ||
| RX J2129+0005 | 0.234 | 322.416 | 0.089 | 14.125 | -34.477 | Y | Y | J | |
| MACS J0429.6-0253 | 0.399 | 67.400 | -2.885 | -24.390 | -32.588 | Y | K | ||
| MACS J1115.9+0129 | 0.352 | 168.966 | 1.499 | -2.987 | 55.625 | Y | K | ||
| MACS J1311.0-0310 | 0.494 | 197.757 | -3.178 | 4.030 | 59.328 | Y | K | ||
| MACS J1931.8-2634 | 0.352 | 292.957 | -26.576 | -4.755 | -20.093 | Y | Y | K | |
| Abell 1489 | 0.350 | 183.079 | 27.553 | 26.318 | 81.304 | Zitrin et al. (2020) | |||
| Abell 1689 | 0.187 | 197.873 | -1.3411 | 35.291 | 61.124 | Y | Limousin et al. (2007) | ||
| PLCK G165.7+67.0 | 0.351 | 171.810 | 42.474 | 35.291 | 67.006 | Frye et al. (2024) |
Notes. We list equatorial coordinates, ecliptic (β) and galactic (b) latitudes, as well as two conditions: whether the cluster has an ecliptic latitude |β|> 54°, which is one of the HLTDS requirements, and whether the cluster falls within LSST observing fields. A - The cluster was studied and modeled by the RELICS program (Cerny et al. 2018; Salmon et al. 2020), but no paper has been published on the cluster. B - The cluster can be observed by the HLTDS if the condition is relaxed to |β|> 50°. C - Cerny et al. (2018). D - Cibirka et al. (2018). E - Acebron et al. (2018). F - the two parts of the cluster were modeled separately. G - Richard et al. (2021). H - Thai et al. (2023). I - The cluster was studied and modeled by Richard et al. (2021) and Thai et al. (2023), but was not included in the papers. Data available at: https://cral-perso.univ-lyon1.fr/labo/perso/johan.richard/MUSE_data_release/, date of access: 2024-04-16. J - Zitrin et al. (2015). K - Caminha et al. (2019).
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