Table 1.
Continuum detections at S/N ≥ 4.5.
| ID | RAJ2000 | DecJ2000 | S/N | S1.1 mm, peak | S1.1 mm,uv−fit | z |
|---|---|---|---|---|---|---|
| (hh:mm:ss.ss) | (±dd:mm:ss.ss) | (mJy beam−1) | (mJy) | |||
| A2744-ID01a | 00:14:19.80 | −30:23:07.66 | 25.9 | 1.433 ± 0.056 | 1.570 ± 0.073 | 2.9c |
| A2744-ID02a | 00:14:18.25 | −30:24:47.47 | 14.4 | 1.292 ± 0.091 | 2.816 ± 0.229 | 2.482c |
| A2744-ID03a | 00:14:20.40 | −30:22:54.42 | 13.9 | 0.798 ± 0.058 | 1.589 ± 0.125 |
d |
| A2744-ID04a | 00:14:17.58 | −30:23:00.56 | 13.8 | 0.932 ± 0.068 | 1.009 ± 0.074 |
d |
| A2744-ID05a | 00:14:19.12 | −30:22:42.20 | 7.7 | 0.655 ± 0.086 | 1.113 ± 0.135 |
d |
| A2744-ID06a | 00:14:17.28 | −30:22:58.60 | 6.5 | 0.574 ± 0.089 | 1.283 ± 0.241 |
d |
| A2744-ID07a | 00:14:22.10 | −30:22:49.67 | 6.2 | 0.455 ± 0.074 | 0.539 ± 0.082 |
d |
| A2744-ID08b | 00:14:24.73 | −30:24:34.20 | 4.8 | 0.270 ± 0.056 | … | … |
| A2744-ID09b | 00:14:21.23 | −30:23:28.70 | 4.7 | 0.256 ± 0.055 | … | … |
| A2744-ID10b | 00:14:17.72 | −30:23:02.25 | 4.5 | 0.286 ± 0.063 | … | … |
| A2744-ID11b | 00:14:22.63 | −30:23:30.45 | 4.5 | 0.253 ± 0.056 | … | … |
| MACS J0416-ID01a | 04:16:10.79 | −24:04:47.53 | 15.4 | 1.010 ± 0.066 | 1.319 ± 0.103 | 2.086c |
| MACS J0416-ID02a | 04:16:06.96 | −24:03:59.96 | 6.8 | 0.406 ± 0.062 | 0.574 ± 0.132 | 1.953c |
| MACS J0416-ID03a | 04:16:08.81 | −24:05:22.58 | 5.8 | 0.389 ± 0.067 | 0.411 ± 0.072 |
d |
| MACS J0416-ID04a | 04:16:11.67 | −24:04:19.44 | 5.1 | 0.333 ± 0.066 | 0.478 ± 0.166 |
d |
| MACS J0416-ID05b | 04:16:10.52 | −24:05:04.77 | 4.6 | 0.302 ± 0.066 | … | 1.849e |
| MACS J1149-ID01a | 11:49:36.09 | +22:24:24.60 | 5.9 | 0.442 ± 0.074 | 0.579 ± 0.134 | 1.46c |
| MACS J1149-ID02b | 11:49:40.32 | +22:24:42.00 | 4.6 | 0.524 ± 0.113 | … | … |
| MACS J1149-ID03b | 11:49:35.41 | +22:23:38.60 | 4.5 | 0.326 ± 0.072 | … | … |
Notes. Column 1: Source ID. Columns 2, 3: Centroid J2000 position of ID. Column 4: Signal-to-noise of the detection. Column 5: PB-corrected peak intensity and 1σ error. Column 6: PB-corrected integrated flux density and 1σ error from uv fitting. Column 7: Source redshift.
Low-significance (4.5 ≤ S/N < 5) detections. Instead of performing a uv fitting, we estimate the integrated flux density using the peak intensity and assuming given source size parameters (see Sect. 2.1.2). Since all but one of them lack clear counterparts (partly due to contamination) and spectroscopic redshifts, nor were they included in Paper II study, we assume a Gaussian redshift distribution with mean z = 2 and σ = 0.5 for these sources.
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