Table B.1.
Characteristics of the continuum-detected target sources.
| Name | RA | Dec | Freq. | S/N | S/N | Sν | νLν | LIR |
|---|---|---|---|---|---|---|---|---|
| (h:min:s) | (deg:min:s) | (GHz) | (tap.) | (μJy) | log10(L/L⊙) | |||
| DEIMOS_COSMOS_873756 | 10:00:02.72 | +02:37:39.99 | 347.4 | 21.7 | 20.1 | 1355 ± 76 | 11.41 | 12.26 |
| DEIMOS_COSMOS_818760 | 10:01:54.86 | +02:32:31.43 | 347.2 | 9.5 | 9.6 | 1077 ± 130 | 11.31 | 12.16 |
| DEIMOS_COSMOS_488399 | 10:03:01.15 | +02:02:35.77 | 291.5 | 9.3 | 9.0 | 253 ± 32 | 10.83 | 11.67 |
| DEIMOS_COSMOS_494057 | 09:58:28.50 | +02:03:06.42 | 295.7 | 7.1 | 5.6 | 179 ± 30 | 10.66 | 11.51 |
| DEIMOS_COSMOS_848185 | 10:00:21.50 | +02:35:11.03 | 307.6 | 7.1 | 7.5 | 319 ± 50 | 10.88 | 11.73 |
| vuds_cosmos_5100822662 | 09:58:57.90 | +02:04:51.38 | 349.8 | 6.5 | 4.8 | 210 ± 38 | 10.60 | 11.45 |
| vuds_cosmos_5101218326 | 10:01:12.50 | +02:18:52.37 | 348.1 | 6.5 | 6.3 | 462 ± 79 | 10.95 | 11.79 |
| vuds_cosmos_5180966608 | 10:01:37.48 | +02:08:23.39 | 350.4 | 5.7 | 5.6 | 419 ± 84 | 10.90 | 11.74 |
| DEIMOS_COSMOS_396844 | 10:00:59.65 | +01:53:47.52 | 348.0 | 5.6 | 4.6 | 346 ± 69 | 10.82 | 11.67 |
| CANDELS_GOODSS_19 | 03:32:22.97 | −27:46:29.32 | 350.6 | 5.4 | 3.9 | 278 ± 61 | 10.71 | 11.57 |
| DEIMOS_COSMOS_683613 | 10:00:09.41 | +02:20:13.41 | 295.8 | 5.1 | 5.1 | 245 ± 54 | 10.80 | 11.65 |
| DEIMOS_COSMOS_552206 | 09:58:26.80 | +02:08:26.80 | 296.7 | 4.5 | 4.5 | 285 ± 73 | 10.86 | 11.71 |
| vuds_cosmos_5101209780 | Multi-component object, see Appendix D.1 | |||||||
| DEIMOS_COSMOS_422677 | 10:01:59.46 | +01:56:12.93 | 355.9 | 4.3 | 3.2 | 375 ± 123 | 10.84 | 11.68 |
| vuds_cosmos_5100969402 | 10:01:20.11 | +02:17:01.13 | 346.0 | 4.0 | 3.9 | 327 ± 99 | 10.80 | 11.65 |
| vuds_cosmos_5100994794 | 10:00:41.18 | +02:17:14.27 | 346.0 | 4.0 | 2.3 | 117 ± 36 | 10.35 | 11.20 |
| CANDELS_GOODSS_32 | 03:32:17.01 | −27:41:13.97 | 356.2 | 3.9 | 3.2 | 230 ± 65 | 10.62 | 11.47 |
| DEIMOS_COSMOS_460378 | 10:00:11.39 | +01:59:54.00 | 302.3 | 3.8 | 2.8 | 116 ± 35 | 10.46 | 11.31 |
| DEIMOS_COSMOS_539609 | 09:59:07.25 | +02:07:21.02 | 314.5 | 3.7 | 3.2 | 187 ± 54 | 10.64 | 11.48 |
| vuds_efdcs_530029038 | Multi-component object, see Appendix D.1 | |||||||
| DEIMOS_COSMOS_493583 | 10:00:23.36 | +02:03:04.23 | 349.4 | 3.6 | 2.9 | 235 ± 81 | 10.64 | 11.50 |
| DEIMOS_COSMOS_417567 | 10:02:04.14 | +01:55:43.93 | 289.9 | 3.6 | 3.7 | 201 ± 60 | 10.73 | 11.58 |
| DEIMOS_COSMOS_881725 | Multi-component object, see Appendix D.1 | |||||||
Notes. The frequency is the mean of the channels used to derive the continuum. The flux Sν was measured using the 2D-fit approached described in Sect. 3.1. The monochromatic luminosity νLν is derived at (1 + z) νobs and does not need any assumption on the galaxy SEDs. The total infrared luminosity LIR (8−1000 μm) is derived assuming Bethermin et al. (2017) SED (see discussion in Sect. 4). The measurement uncertainties do not include the calibration uncertainties (∼4.5% on average and up to 10%, see Sect. 2.3).
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