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Table 1
The sample of spectroscopically confirmed z> 4 SMGs in the COSMOS field.
| Source | α 2000.0 | δ 2000.0 | z spec | S λ | λ | Instruments |
| [°] | [°] | [mJy] | [mm] | |||
|
|
||||||
| AzTEC1 | 149.92859 | 2.49394 | 4.640 | 9.3 ± 1.3 | 1.1 | JCMT/AzTEC, SMA, Keck II/DEIMOS |
| AzTEC3 | 150.08624 | 2.58903 | 5.298 | 5.9 ± 1.3 | 1.1 | JCMT/AzTEC, SMA, Keck II/DEIMOS |
| AzTEC/C159 | 149.87671 | 1.92432 | 4.569 | 3.3 ± 1.3 | 1.1 | ASTE/AzTEC,VLA, Keck II/DEIMOS |
| J1000+0234 | 150.22717 | 2.57644 | 4.542 | 3.4 ± 0.7 | 1.2 | IRAM-30 m/MAMBO, PdBI, Keck II/DEIMOS |
| Vd-17871 | 150.36284 | 2.14883 | 4.622 | 2.5 ± 0.5 | 1.2 | IRAM-30 m/MAMBO, PdBI, Keck II/DEIMOS, VLT/VIMOS |
| AK03 | 150.07841 | 2.47061 | 4.747 | 11.42 ± 4.98 | 0.450 | JCMT/SCUBA2, VLA, Keck II/DEIMOS |
Notes. Column 6 gives the (sub)mm-wavelength used for initial identification of the source as an SMG, and the last column lists the instruments used for initial (sub)mm-detection, and counterpart and redshift association.
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