Table 1
Galaxy overdensities hosting SMGs in order of increasing redshift.
| Field or source ID | z | Reference |
|
|
||
| Cosbo-16a | 1.4 | Aravena et al. (2010) |
| XCS J2215.9-1738 | 1.46 | Ma et al. (2015) |
| Cosbo-6 | 1.6 | Aravena et al. (2010) |
| GOODS-N | 1.99 | Chapman et al. (2009) |
| MRC1138-262 | 2.16 | Dannerbauer et al. (2014) |
| Cosbo-3b | 2.3 | Aravena et al. (2010); Casey et al. (2015) |
| 53W002 | 2.39 | Smail et al. (2003) |
| SSA22 | 3.09 | Chapman et al. (2001); Tamura et al. (2009) |
| 4C+41.17 | 3.8 | Ivison et al. (2000); Stevens et al. (2003) |
| GN20/20.2 | 4.05 | Daddi et al. (2009) |
| HDF850.1 | 5.2 | Walter et al. (2012) |
| AzTEC3b | 5.3 | Capak et al. (2011) |
Notes.
The association of the target SMG (Cosbo-16) with the z ~ 1.4 overdensity is uncertain because of the uncertainty in the photometric redshift of the SMG.
The Cosbo-3 and AzTEC3 systems are analysed in the present study. We note that we use the revised spectroscopic redshift of zspec = 2.49 for Cosbo-3 (Wang et al. 2016; D. A. Riechers et al., in prep.; see also Smolčić et al. 2012b).
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