Table 10.
Protoclusters from the literature at 1.9 < z < 2.6.
| Name | Redshift | N | Selection | ΣSFR | Reference |
|---|---|---|---|---|---|
| members (a) | method (b) | (M⊙ yr−1) | |||
| CARLA J1018+0530 | 1.952 | 8 | HzRG | 512 | (1) |
| CARLA J0800+4029 | 1.985 | 9 | HzRG | 754 | (1) |
| Cl J1449+0856 | 1.990 | 15 | phot | 1236 | (2,3) |
| CARLA J2039−2514 | 1.999 | 9 | HzRG | 945 | (1) |
| ZFIRE | 2.085 | 9 | phot | 4002 | (4) |
| MRC 1138−262 | 2.157 | 36 | HzRG | 5713 | (5,6,7) |
| PHz G237.01+42.50 ss1 | 2.155 | 20 | sub-mm | 1002 | (this work) |
| HELAISS02 | 2.170 | 4 | sub-mm | 1492 | (8) |
| 2QZCluster | 2.230 | 7 | sub-mm | 2004 | (9) |
| CC2.2 | 2.233 | 40 | HAE | 2228 | (10) |
| HS 1700+64 | 2.310 | 13 | sub-mm | 5290 | (9,11,12) |
| HATLAS J084933 | 2.412 | 4 | sub-mm | 6026 | (13) |
| PCL 1002 | 2.472 | 41 | sub-mm | 4447 | (14) |
| 4C 23.56 | 2.488 | 27 | HzRG | 3887 | (6,15) |
| CL J1001 | 2.507 | 14 | phot | 2790 | (16) |
| USS 1558−003 | 2.528 | 35 | HzRG | 2375 | (6) |
| HXMM20 | 2.609 | 5 | sub-mm | 1877 | (8) |
Notes.
The listed protoclusters have been found through the following methods, HzRG: search around a HzRG, phot: identification of an overdensity of photometrically selected high-z sources, sub-mm: overdensity of sub-mm sources, HAE: overdensity of Hα emitters in narrowband images.
References. (1) Noirot et al. (2018), (2) Smith et al. (2019), (3) Valentino et al. (2015), (4) Hung et al. (2016), (5) Dannerbauer et al. (2017), (6) Tadaki et al. (2019), (7) Hatch et al. (2009), (8) Gómez-Guijarro et al. (2019), (9) Kato et al. (2016), (10) Darvish et al. (2020), (11) Lacaille et al. (2019), (12) Chapman et al. (2015), (13) Ivison et al. (2013), (14) Casey et al. (2015), (15) Lee et al. (2017), (16) Wang et al. (2018).
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