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Table 4.
Deblended SCUBA-2 and Herschel-SPIRE flux densities for the individual ALMA-detected galaxies.
| ID | S250 | S350 | S500 | S850 |
|---|---|---|---|---|
| (mJy) | (mJy) | (mJy) | (mJy) | |
| 0 | 71 |
48 |
22 |
4.7 |
| 1 | 19 |
29 |
23 |
7.8 |
| 2 | < 12 | 10 |
10 |
4.3 |
| 3 | 25 |
25 |
16 |
4.6 |
| 4 | 31 |
16 |
6 |
1.0 |
| 5 | 21 |
25 |
17 |
5.0 |
| 6 | 14 |
11 |
6 |
1.4 |
| 7 | 9 |
9 |
5 |
1.3 |
| 8 | 64 |
43 |
20 |
4.2 |
| 9 | < 8 | 6 |
7 |
2.8 |
| 10 | 46 |
35 |
17 |
3.9 |
| 11 | < 32 | < 41 | < 13 | 2.7 |
| 12 | 28 |
22 |
12 |
2.8 |
| 13 | 9 |
16 |
14 |
5.1 |
| 14 | 18 |
18 |
10 |
2.7 |
| 15 | < 1.4 | < 5 | < 7 | 1.3 |
| 16 | < 1.3 | < 4 | < 6 | < 2.4 |
| 17 | 40 |
24 |
10 |
1.9 |
Notes. In cases where the measured flux density is < 2σ, we report an upper limit corresponding to the maximum likelihood flux density plus 3σ.
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