Table 2.
Continuum fluxes for the RS NIR-dark galaxies analysed in this study.
| ID | S3 mm | S850 μm | Other flux |
|---|---|---|---|
| [mJy] | [mJy] | [mJy] | |
| 41 | (0.04 ± 0.01) | (2.9 ± 0.3) | – |
| 84 | (0.11 ± 0.03) | (7 ± 2) | 0.873 mm: (4.6 ± 0.8) |
| 121 | (0.09 ± 0.03) | (3.9 ± 0.4) | – |
| 182 | (0.14 ± 0.02) | (5 ± 1) | – |
| 235 | (0.18 ± 0.04) | (5 ± 1) | – |
| 247 | (0.09 ± 0.01) | (5 ± 1) | – |
| 298 | < 0.036 | (3.3 ± 0.3) | – |
| 361 | < 0.036 | (3.3 ± 0.4) | 1.249 mm: (2.0 ± 0.4) |
| 456 | < 0.036 | (1.9 ± 0.2) | – |
Notes. The values at λ = 3 mm are obtained through aperture photometry on the continuum images obtained in Sect. 3.1. We consider a source as robustly detected with a S/N > 3, and therefore, we report a 3σ upper limit for the undetected targets. The value at 850 μm is retrieved from the SuperDeblended catalog (Jin et al. 2018) for the sources at S/N > 3 (reported in bold), while for the other galaxies, we report the best-fitting flux at 850 μm computed with CIGALE. For two sources, we also report an additional (sub)mm flux measured with ALMA through cross-matching with the A3COSMOS catalog (Liu et al. 2019).
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