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Table C.1.
X-CLASS clusters spectroscopically confirmed with SPIDERS (see Sect. 4.1.3).
| Xclass | Nz | Obs. status | Nmem | Zspec | Xclass | Nz | Obs. status | Nmem | Zspec |
|---|---|---|---|---|---|---|---|---|---|
| 0039 | 12 | Complete | 7 | 0.2810 ± 0.0009 | 1624 | 15 | Complete | 12 | 0.2276 ± 0.0009 |
| 0040 | 15 | Complete | 12 | 0.3274 ± 0.0009 | 1626 | 5 | Complete | 5 | 0.548 ± 0.002 |
| 0062 | 18 | Complete | 18 | 0.362 ± 0.002 | 1627 | 16 | Complete | 15 | 0.3297 ± 0.0009 |
| 0096 | 17 | Complete | 16 | 0.252 ± 0.001 | 1635 | 11 | Complete | 8 | 0.428 ± 0.001 |
| 0099 | 26 | Complete | 22 | 0.2311 ± 0.0007 | 1637 | 24 | Complete | 22 | 0.206 ± 0.001 |
| 0102 | 15 | Complete | 14 | 0.0593 ± 0.0003 | 1642 | 14 | Complete | 9 | 0.55 ± 0.01 |
| 0103 | 12 | Complete | 11 | 0.1320 ± 0.0005 | 1674 | 17 | Complete | 8 | 0.580 ± 0.001 |
| 0108 | 19 | Complete | 14 | 0.1949 ± 0.0006 | 1676 | 27 | Complete | 14 | 0.2881 ± 0.0004 |
| 0109 | 12 | Complete | 9 | 0.478 ± 0.001 | 1678 | 24 | Complete | 18 | 0.409 ± 0.002 |
| 0110 | 24 | Complete | 14 | 0.2703 ± 0.0009 | 1680 | 4 | Complete | 3 | 0.552 ± 0.004 |
| 0169 | 10 | Complete | 9 | 0.320 ± 0.002 | 1686 | 11 | Complete | 6 | 0.3076 ± 0.0009 |
| 0224 | 15 | Complete | 11 | 0.1423 ± 0.0006 | 1706 | 9 | Incomplete | 6 | 0.3321 ± 0.0004 |
| 0245 | 10 | Complete | 7 | 0.1603 ± 0.0003 | 1737 | 21 | Complete | 20 | 0.276 ± 0.001 |
| 0270 | 15 | Complete | 12 | 0.2452 ± 0.0006 | 1738 | 20 | Complete | 18 | 0.280 ± 0.002 |
| 0336 | 17 | Complete | 13 | 0.421 ± 0.001 | 1758 | 7 | Complete | 6 | 0.342 ± 0.001 |
| 0342 | 4 | Incomplete | 3 | 0.230 ± 0.003 | 1763 | 9 | Complete | 4 | 0.3124 ± 0.0006 |
| 0343 | 17 | Incomplete | 15 | 0.351 ± 0.001 | 1764 | 15 | Complete | 8 | 0.311 ± 0.001 |
| 0344 | 14 | Complete | 11 | 0.2909 ± 0.0006 | 1789 | 10 | Complete | 2 | 0.59(1) |
| 0347 | 3 | Incomplete | 2 | 0.26(1) | 1807 | 16 | Complete | 10 | 0.4999 ± 0.0006 |
| 0349 | 28 | Complete | 22 | 0.1537 ± 0.0005 | 1816 | 10 | Complete | 3 | 0.579 ± 0.001 |
| 0361 | 8 | Complete | 7 | 0.0454 ± 0.0007 | 1817 | 9 | Complete | 5 | 0.579 ± 0.002 |
| 0377 | 9 | Incomplete | 8 | 0.395 ± 0.002 | 1853 | 33 | Complete | 26 | 0.2972 ± 0.0008 |
| 0574 | 8 | Complete | 4 | 0.497 ± 0.002 | 1854 | 14 | Complete | 8 | 0.519 ± 0.001 |
| 0578 | 30 | Complete | 29 | 0.1396 ± 0.0007 | 1855 | 11 | Complete | 8 | 0.1865 ± 0.0007 |
| 0615 | 11 | Complete | 6 | 0.255 ± 0.001 | 1866 | 2 | Complete | 2 | 0.44(1) |
| 0628 | 7 | Complete | 6 | 0.2323 ± 0.0006 | 1900 | 13 | Complete | 8 | 0.413 ± 0.002 |
| 0630 | 5 | Complete | 4 | 0.373 ± 0.001 | 1904 | 34 | Complete | 32 | 0.0895 ± 0.0003 |
| 0632 | 19 | Complete | 14 | 0.3947 ± 0.0005 | 1941 | 17 | Complete | 14 | 0.0996 ± 0.0003 |
| 0638 | 6 | Complete | 4 | 0.500 ± 0.001 | 1957 | 23 | Complete | 23 | 0.2696 ± 0.0009 |
| 0686 | 8 | Complete | 4 | 0.460 ± 0.003 | 1982 | 10 | Complete | 6 | 0.248 ± 0.001 |
| 0706 | 5 | Complete | 4 | 0.609 ± 0.002 | 1983 | 10 | Complete | 9 | 0.3453 ± 0.0004 |
| 0734 | 6 | Complete | 4 | 0.427 ± 0.004 | 2003 | 7 | Complete | 5 | 0.532 ± 0.003 |
| 0740 | 14 | Complete | 9 | 0.3388 ± 0.0008 | 2026 | 8 | Complete | 4 | 0.527 ± 0.001 |
| 0755 | 18 | Complete | 14 | 0.1969 ± 0.0004 | 2034 | 6 | Incomplete | 5 | 0.248 ± 0.001 |
| 0841 | 13 | Complete | 7 | 0.551 ± 0.003 | 2036 | 13 | Complete | 6 | 0.328 ± 0.001 |
| 0842 | 29 | Complete | 22 | 0.3009 ± 0.0009 | 2051 | 17 | Complete | 9 | 0.411 ± 0.002 |
| 0890 | 19 | Complete | 13 | 0.3397 ± 0.0007 | 2080 | 11 | Complete | 6 | 0.427 ± 0.002 |
| 0908 | 16 | Complete | 11 | 0.2744 ± 0.0005 | 2081 | 21 | Complete | 19 | 0.293 ± 0.002 |
| 0953 | 12 | Complete | 7 | 0.1327 ± 0.0002 | 2088 | 13 | Complete | 11 | 0.0900 ± 0.0009 |
| 0963 | 13 | Complete | 12 | 0.2477 ± 0.0005 | 2090 | 26 | Complete | 25 | 0.0904 ± 0.0006 |
| 1013 | 10 | Complete | 8 | 0.4149 ± 0.0005 | 2093 | 21 | Complete | 16 | 0.2970 ± 0.0008 |
| 1059 | 26 | Complete | 22 | 0.2791 ± 0.0005 | 2097 | 19 | Complete | 18 | 0.1125 ± 0.0006 |
| 1062 | 26 | Complete | 22 | 0.1238 ± 0.0004 | 2109 | 25 | Complete | 20 | 0.2128 ± 0.0006 |
| 1069 | 9 | Complete | 9 | 0.1328 ± 0.0004 | 2154 | 8 | Complete | 7 | 0.329 ± 0.001 |
| 1086 | 7 | Complete | 7 | 0.423 ± 0.002 | 2155 | 9 | Complete | 8 | 0.390 ± 0.001 |
| 1159 | 22 | Complete | 20 | 0.412 ± 0.001 | 2182 | 6 | Complete | 6 | 0.520 ± 0.002 |
| 1185 | 11 | Complete | 5 | 0.492 ± 0.002 | 2208 | 13 | Complete | 8 | 0.1050 ± 0.0004 |
| 1288 | 18 | Complete | 13 | 0.532 ± 0.002 | 2214 | 20 | Complete | 15 | 0.3004 ± 0.0004 |
| 1307 | 28 | Complete | 26 | 0.0593 ± 0.0004 | 2272 | 13 | Complete | 9 | 0.254 ± 0.003 |
| 1350 | 4 | Incomplete | 3 | 0.396 ± 0.001 | 2295 | 28 | Complete | 22 | 0.3695 ± 0.0007 |
| 1351 | 11 | Incomplete | 6 | 0.543 ± 0.002 | 2328 | 2 | Complete | 2 | 0.45(1) |
| 1368 | 23 | Complete | 20 | 0.288 ± 0.001 | 2338 | 31 | Complete | 29 | 0.1406 ± 0.0004 |
| 1369 | 12 | Complete | 5 | 0.284 ± 0.002 | 2340 | 12 | Complete | 11 | 0.443 ± 0.002 |
| 1386 | 13 | Complete | 12 | 0.314 ± 0.001 | 2344 | 21 | Complete | 21 | 0.232 ± 0.002 |
| 1439 | 23 | Complete | 21 | 0.0573 ± 0.0006 | 2345 | 22 | Complete | 20 | 0.219 ± 0.001 |
| 1443 | 31 | Complete | 24 | 0.0543 ± 0.0006 | 2347 | 28 | Complete | 26 | 0.1672 ± 0.0007 |
| 1451 | 8 | Complete | 6 | 0.478 ± 0.004 | 2348 | 26 | Complete | 25 | 0.1921 ± 0.0009 |
| 1452 | 7 | Complete | 5 | 0.447 ± 0.004 | 2350 | 23 | Complete | 20 | 0.412 ± 0.001 |
| 1543 | 10 | Complete | 10 | 0.370 ± 0.001 | 2353 | 25 | Complete | 23 | 0.190 ± 0.001 |
| 1544 | 19 | Complete | 18 | 0.370 ± 0.001 | 2358 | 30 | Complete | 25 | 0.0949 ± 0.0007 |
| 1548 | 5 | Complete | 5 | 0.3281 ± 0.0006 | 2360 | 14 | Complete | 10 | 0.235 ± 0.002 |
| 1622 | 21 | Complete | 14 | 0.0794 ± 0.0003 | 2363 | 14 | Complete | 8 | 0.312 ± 0.002 |
Notes. This table lists the systems that are validated with Nmem spectroscopic redshifts selected among Nz redshifts available in their red sequence. The observational status indicates ‘complete’ if all selected targets led to a spectrum acquisition. The spectroscopic redshift uncertainty reflects the spread in the Nmem redshift values. A few systems marked with (1) were confirmed with only two spectroscopic members, hence no uncertainty is given on the redshift.
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