Table A.1
Median stacked fluxes derived in each redshift bin through a bootstrapping procedure.
| Redshift bin | N stack | PACS 100 | PACS 160 | SPIRE 250 | SPIRE 350 | SPIRE 500 |
| [mJy] | [mJy] | [mJy] | [mJy] | [mJy] | ||
|
|
||||||
| 0.01 ≤ z< 0.30 | 37 | <0.42 | 1.90 |
2.20 |
2.24 |
<3.02 |
| 0.30 ≤ z< 0.70 | 366 | 1.09 |
2.22 |
1.64 |
0.89 |
<1.09 |
| 0.70 ≤ z< 1.20 | 642 | 1.02 |
1.91 |
1.98 |
1.47 |
0.70 |
| 1.20 ≤ z< 1.80 | 620 | 1.44 |
3.03 |
4.21 |
4.25 |
2.75 |
| 1.80 ≤ z< 2.50 | 306 | 0.95 |
2.49 |
3.33 |
3.77 |
3.10 |
| 2.50 ≤ z< 3.50 | 175 | 1.00 |
2.25 |
5.44 |
5.73 |
4.55 |
| 3.50 ≤ z< 5.70 | 57 | 0.79 |
2.15 |
5.19 |
7.68 |
6.80 |
Notes. Lower and upper errors (in mJy) correspond to the 16th and 84th percentiles of the cumulative flux distribution. In case the error is larger than the median flux, we report the 1σ upper flux. The number of stacked sources Nstack is reported for each redshift bin.
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