Table 2.
Summary of the photometry derived in this work.
| z bin | log M⋆ bin | Nobj | Flux density | erFluxstack | erFluxind | erFluxtotal |
|---|---|---|---|---|---|---|
| (M⊙) | (μJy) | (μJy) | (μJy) | (μJy) | ||
| Whole | Sample | |||||
| 8 ≤ log M⋆ < 9 | 910 | < 17.31 | – | – | – | |
| 1.0 ≤ z < 1.5 | 9 ≤ log M⋆ < 10 | 299 | < 25.88 | – | – | – |
| 10 ≤ log M⋆ ≤ 11 | 92 | 132.10 | 20.36 | 21.55 | 29.65 | |
| 8 ≤ log M⋆ < 9 | 1423 | < 12.70 | – | – | – | |
| 1.5 ≤ z < 2.0 | 9 ≤ log M⋆ < 10 | 353 | < 26.13 | – | – | – |
| 10 ≤ log M⋆ ≤ 11 | 96 | 148.31 | 18.67 | 24.49 | 30.79 | |
| 8 ≤ log M⋆ < 9 | 881 | < 14.99 | – | – | – | |
| 2.0 < z < 2.5 | 9 ≤ log M⋆ < 10 | 274 | < 25.94 | – | – | – |
| 10 ≤ log M⋆ ≤ 11 | 54 | 219.30 | 24.01 | 25.33 | 34.90 | |
| 8 ≤ log M⋆ < 9 | 751 | < 15.71 | – | – | – | |
| 2.5 ≤ z ≤ 3.0 | 9 ≤ log M⋆ < 10 | 340 | < 26.38 | – | – | – |
| 10 ≤ log M⋆ ≤ 11 | 57 | 211.26 | 24.79 | 47.62 | 53.69 | |
| Undetected | Sources | |||||
| 8 ≤ log M⋆ < 9 | 890 | < 16.83 | – | – | – | |
| 1.0 ≤ z < 1.5 | 9 ≤ log M⋆ < 10 | 285 | < 25.71 | – | – | – |
| 10 ≤ log M⋆ ≤ 11 | 85 | 115.97 | 20.91 | 20.84 | 29.52 | |
| 8 ≤ log M⋆ < 9 | 1387 | < 11.75 | – | – | ||
| 1.5 ≤ z < 2.0 | 9 ≤ log M⋆ < 10 | 338 | < 25.57 | – | – | – |
| 10 ≤ log M⋆ ≤ 11 | 84 | 110.66 | 19.72 | 22.06 | 29.59 | |
| 8 ≤ log M⋆ < 9 | 854 | < 14.64 | – | – | – | |
| 2.0 < z < 2.5 | 9 ≤ log M⋆ < 10 | 265 | < 30.55 | – | – | – |
| 10 ≤ log M⋆ ≤ 11 | 46 | 165.87 | 24.83 | 29.67 | 38.69 | |
| 8 ≤ log M⋆ < 9 | 732 | < 14.86 | – | – | – | |
| 2.5 ≤ z ≤ 3.0 | 9 ≤ log M⋆ < 10 | 325 | < 27.91 | – | – | – |
| 10 ≤ log M⋆ ≤ 11 | 47 | 165.93 | 27.05 | 31.84 | 41.78 | |
Notes. We show the flux densities for our sample, and a subsample excluding the Gómez-Guijarro et al. (2022a) sources and those from Guo et al. (2013) which are closer than 5″ to them, as explained in Sect. 2. We split the total uncertainty into its two components: the error due to the stacked data and the uncertainty linked to the underlying distribution of the individual galaxies. The total uncertainty is obtained by summing the previous error contributions in quadrature. The absence of uncertainty denotes an upper limit at the 3σ level.
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