Table 3.
Stacking results in the stellar mass subsamples.
| ⟨z⟩ | log(⟨|M*|⟩/M⊙) | ⟨Dust mass⟩ | Flux | RMS | ⟨μ⟩ (a) |
|---|---|---|---|---|---|
| (M⊙) | (mJy) | (mJy) | |||
| 1.42 | 8.48 | < 2.49 × 106 | – | 4.28 × 10−3 | 3.43 |
| 2.51 | 8.53 | < 1.82 × 106 | – | 5.64 × 10−3 | 5.41 |
| 3.45 | 8.54 | < 1.27 × 106 | – | 6.51 × 10−3 | 7.83 |
| 4.47 | 8.56 | < 9.43 × 105 | – | 6.98 × 10−3 | 10.55 |
| 1.42 | 9.43 | 1.61 × 107 ± 4.33 × 106 | 7.84 × 10−2 | 6.67 × 10−3 | 3.24 |
| 2.54 | 9.39 | 3.89 × 106 ± 2.54 × 106 | 2.54 × 10−2 | 8.25 × 10−3 | 3.78 |
| 3.41 | 9.41 | 4.96 × 106 ± 2.61 × 106 | 4.49 × 10−2 | 9.12 × 10−3 | 4.64 |
| 4.44 | 9.42 | < 2.19 × 106 | – | 9.12 × 10−3 | 5.95 |
| 1.41 | 10.42 | 6.95 × 107 ± 1.84 × 107 | 0.28 | 1.27 × 10−2 | 2.67 |
| 2.46 | 10.33 | 5.57 × 107 ± 1.78 × 107 | 0.3 | 2.37 × 10−2 | 3.16 |
| 3.43 | 10.35 | 3.57 × 107 ± 1.32 × 107 | 0.33 | 1.96 × 10−2 | 4.71 |
| 4.46 | 10.37 | 1.7 × 107 ± 1.01 × 107 | 0.2 | 2.02 × 10−2 | 5.67 |
| 1.41 | 11.2 | 1.02 × 108 ± 4.17 × 107 | 0.39 | 2.88 × 10−2 | 2.53 |
| 2.56 | 11.22 | < 3.58 × 107 | – | 9.51 × 10−2 | 4.6 |
| 3.55 | 11.38 | < 3.21 × 107 | – | 4.93 × 10−2 | 2.33 |
| 4.46 | 11.39 | 1.55 × 107 ± 1.11 × 107 | 0.16 | 4.03 × 10−2 | 4.87 |
Notes. When the central flux is lower than three times the RMS of the corresponding stack map, the 3 σ upper limit is shown in place of the dust mass. The errors on the computed dust mass correspond to the quadratic sum of the standard deviation computed from empty stacks with the uncertainties from the bootstrap analysis, to which we finally propagated the magnification error (see Sect. 3.4). Flux and RMS are extracted as indicated in Sect. 3.1: The flux is integrated in the central circular region of the stack stamp, with a radius Rinteg = 2″, and it is then converted into Jy from Jy/beam. The RMS is computed from the standard deviation in the empty stacks.
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