Table 4
Statistical samples of SMGs with ≲2′′ angular resolution mm-detections in the COSMOS field.
| 1.1 mm-selected | Best | Least-biased- | Best |
| sample | redshift | 870 μm-selected | redshift |
| sample | |||
|
|
|||
| AzTEC-1 | 4.64+ | COSLA-1 |
*
|
| AzTEC-2 | 1.125+ | COSLA-2 | 2.490+ |
| AzTEC-3 | 5.299+ | COSLA-3 | 1.357+ |
| AzTEC-4 |
#
|
COSLA-4 | 1.125+ |
| AzTEC-5 | 3.971+ | COSLA-6-N |
*
|
| AzTEC-6 | 0.802+ | COSLA-6-S |
|
| AzTEC-7 | 2.30 ± 0.10 | COSLA-17-S |
|
| AzTEC-8 | 3.179+ | COSLA-17-N |
#
|
| AzTEC-9 | 1.357+ | COSLA-23-N |
#
|
| AzTEC-10 |
|
COSLA-23-S |
|
| AzTEC-11** | 1.599+ | COSLA-47 |
|
| AzTEC-11N** |
|
COSLA-54 |
|
| AzTEC-11S** | >2.58 | COSLA-60 | 4.64+ |
| AzTEC-12 |
|
COSLA-73 | 3.179+ |
| AzTEC-13 | >3.59* | COSLA-128 |
|
| AzTEC-14-E | >3.03* | COSLA-158 | >3.59* |
| AzTEC-14-W |
|
||
| AzTEC-15 |
#
|
||
Notes. Five SMGs belong to both samples; AzTEC-1/COSLA-60, AzTEC-2/COSLA-4, AzTEC-8/COSLA-73, AzTEC-9/COSLA-3, AzTEC-13/COSLA-158.
Here we keep the nomenclature given by Younger et al. (2009). Note however that AzTEC-11-S is the northern component of the AzTEC-11 SMG, and AzTEC-11-N is its southern component (see Table 1 in Younger et al. 2009).
Spectroscopic redshift (see Table 1 for references).
Photometric redshift corrected for the systematic offset of 0.04(1 + z), see Fig. 6, with errors drawn from the total χ2 distribution.
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