Table 1.
Compilation of protoclusters and high-redshift clusters and groups known in the literature for the COSMOS field.
ID | Name | RA [deg] | Dec [deg] | z | Reference(s) | Matched |
---|---|---|---|---|---|---|
1 | ZFOURGE/ZFIRE | 150.094 | 2.251 | 2.095 | (1), (2) | ✓ |
2 | G237 | 150.507 | 2.312 | 2.160 | (3) | |
311 | – | 150.474 | 2.328 | 2.160 | (4) | ✓ |
315 | – | 150.208 | 2.015 | 2.230 | (5) | ✓ |
3 | CC2.2 | 150.197 | 2.003 | 2.232 | (6) | ✓ |
314 | – | 150.060 | 2.200 | 2.300 | (7) | |
12–16 | COSTCO | [149.706, 150.129] | [2.024, 2.275] | [2.047, 2.391] | (8), (9), (10) | ✓ (100%) |
312 | Colossus | 150.060 | 2.310 | 2.440 | (11), (7), (12), (13) | |
313 | – | 150.130 | 2.373 | 2.470 | (14) | ✓ |
310 | CL J1001+0220 | 150.250 | 2.333 | 2.506 | (15) | ✓ |
5–11 | Hyperion | [149.958, 150.331] | [2.112, 2.404] | [2.423, 2.507] | (16) | ✓ (100%) |
341–345 | LATIS1-D2 | [149.532, 150.347] | [1.988, 2.274] | [2.457, 2.685] | (17) | ✓ (100%) |
91–266 | – | [149.409, 150.749] | [1.628, 2.793] | [2.000, 2.840] | (18) | ✓ (82%) |
4 | QO-1000 | 150.043 | 1.694 | 2.770 | (19) | ( ⊘ ) |
335–340 | – | [149.601, 150.620] | [1.593, 2.289] | [2.010, 2.900] | (20), (21) | ✓ (100%) ( * ) |
316 | VPC-1000 | 150.068 | 1.967 | 2.900 | (22) | ✓ |
17–55 | – | [149.870, 150.588 ] | [1.766, 2.603] | [2.013, 2.957] | (23) | ✓ (82%) |
267–297 | – | [149.509, 150.693] | [1.707, 2.674] | [2.070, 3.080] | (24) | ✓ (92%) |
334 | MAGAZ3NE | 150.429 | 2.506 | 3.120 | (25) | ✓ |
321–326 | – | [149.583, 150.346] | [1.967, 2.603] | [2.194, 3.295] | (26), (27) | ✓ (80%) |
317–320 | CCPC | [149.980, 150.070] | [2.110, 2.280] | [2.098, 3.303] | (28) | ✓ (100%) |
308–309 | MAGAZ3NE | [149.850, 150.117] | [2.333, 2.564] | [3.367, 3.380] | (29) | ✓ (100%) |
298–307 | Elentari | [149.732, 150.424] | [2.275, 2.583] | [3.248, 3.409] | (30) | ✓ (100%) |
56–90 | – | [149.410, 150.616] | [1.543, 2.794] | [2.000, 3.500] | (31) | ✓ (82%) |
327–333 | – | [149.706, 150.751] | [1.798, 2.762] | [2.323, 3.613] | (32) | ( ⋆ ) |
Notes. The table shows arbitrary identification numbers in our compilation (ID), name of the protocluster or the survey, if available (Name), coordinate in degrees or range of coordinates (RA, Dec), redshift or range of redshifts (z), reference(s) and whether or not the objects are matched with one of our detection (and in which fraction if the reference is a catalog or list of objects). ( ⊘ )Outside the COSMOS-Web field; ( ⋆ )all outside the COSMOS-Web field except for one object, which is unmatched; ( * )all outside the COSMOS-Web field except for two objects, both matched. (1) Spitler et al. (2012); (2) Yuan et al. (2014); (3) Polletta et al. (2021); (4) Koyama et al. (2021); (5) Geach et al. (2012); (6) Darvish et al. (2020); (7) Lee et al. (2016); (8) Ata et al. (2022); (9) Dong et al. (2023); (10) Edward et al. (2024); (11) Lee et al. (2014); (12) Diener et al. (2015); (13) Chiang et al. (2015); (14) Casey et al. (2015); (15) Wang et al. (2016); (16) Cucciati et al. (2018); (17) Newman et al. (2022); (18) Sarron & Conselice (2021); (19) Ito et al. (2023); (20) Castignani et al. (2014); (21) Castignani et al. (2019); (22) Cucciati et al. (2014); (23) Diener et al. (2013); (24) Chiang et al. (2014); (25) McConachie et al. (2025); (26) Daddi et al. (2021); (27) Daddi et al. (2022); (28) Franck & McGaugh (2016); (29) McConachie et al. (2022); (30) Forrest et al. (2023); (31) Gozaliasl et al. (in prep.); (32) Sillassen et al. (2024).
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