Table 2.
Continuum detections at S/N ≥ 4.5.
| ID | RAJ2000 | DecJ2000 | S/N | S1.1 mm, peak | S1.1 mm,uv−fit | rs | z |
|---|---|---|---|---|---|---|---|
| (hh:mm:ss.ss) | (±dd:mm:ss.ss) | (mJy beam−1) | (mJy) | (″) | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| A2744-ID01 (a) | 00:14:19.80 | −30:23:07.66 | 25.9 | 1.433 ± 0.056 | 1.570 ± 0.073 | 0.05 ± 0.01 | 2.9 (c) |
| A2744-ID02 (a) | 00:14:18.25 | −30:24:47.47 | 14.4 | 1.292 ± 0.091 | 2.816 ± 0.229 | 0.23 ± 0.04 | 2.585 (d) |
| A2744-ID03 (a) | 00:14:20.40 | −30:22:54.42 | 13.9 | 0.798 ± 0.058 | 1.589 ± 0.125 | 0.26 ± 0.03 | 3.058 (d) |
| A2744-ID04 (a) | 00:14:17.58 | −30:23:00.56 | 13.8 | 0.932 ± 0.068 | 1.009 ± 0.074 | 0.06 ± 0.02 | 1.498 (d) |
| A2744-ID05 (a) | 00:14:19.12 | −30:22:42.20 | 7.7 | 0.655 ± 0.086 | 1.113 ± 0.135 | 0.19 ± 0.05 | 2.409 (d) |
| A2744-ID06 (a) | 00:14:17.28 | −30:22:58.60 | 6.5 | 0.574 ± 0.089 | 1.283 ± 0.241 | 0.26 ± 0.08 |
 (e) |
| A2744-ID07 (a) | 00:14:22.10 | −30:22:49.67 | 6.2 | 0.455 ± 0.074 | 0.539 ± 0.082 | 0.07 ± 0.04 | 2.644 (d) |
| A2744-ID08 (b) | 00:14:24.73 | −30:24:34.20 | 4.8 | 0.270 ± 0.056 | ... | ... | ... |
| A2744-ID09 (b) | 00:14:21.23 | −30:23:28.70 | 4.7 | 0.256 ± 0.055 | ... | ... | ... |
| A2744-ID10 (b) | 00:14:17.72 | −30:23:02.25 | 4.5 | 0.286 ± 0.063 | ... | ... | ... |
| A2744-ID11 (b) | 00:14:22.63 | −30:23:30.45 | 4.5 | 0.253 ± 0.056 | ... | ... | ... |
| MACSJ0416-ID01 (a) | 04:16:10.79 | −24:04:47.53 | 15.4 | 1.010 ± 0.066 | 1.319 ± 0.103 | 0.23 ± 0.06 | 2.086 (c) |
| MACSJ0416-ID02 (a) | 04:16:06.96 | −24:03:59.96 | 6.8 | 0.406 ± 0.062 | 0.574 ± 0.132 | 0.32 ± 0.15 | 1.953 (c) |
| MACSJ0416-ID03 (a) | 04:16:08.81 | −24:05:22.58 | 5.8 | 0.389 ± 0.067 | 0.411 ± 0.072 | 0.10 ± 0.07 |
 (e) |
| MACSJ0416-ID04 (a) | 04:16:11.67 | −24:04:19.44 | 5.1 | 0.333 ± 0.066 | 0.478 ± 0.166 | 0.37 ± 0.21 |
 (e) |
| MACSJ0416-ID05 (b) | 04:16:10.52 | −24:05:04.77 | 4.6 | 0.302 ± 0.066 | ... | ... | 1.849 (f) |
| MACSJ1149-ID01 (a) | 11:49:36.09 | +22:24:24.60 | 5.9 | 0.442 ± 0.074 | 0.579 ± 0.134 | 0.28 ± 0.13 | 1.46 (c) |
| MACSJ1149-ID02 (b) | 11:49:40.32 | +22:24:42.00 | 4.6 | 0.524 ± 0.113 | ... | ... | ... |
| MACSJ1149-ID03 (b) | 11:49:35.41 | +22:23:38.60 | 4.5 | 0.326 ± 0.072 | ... | ... | ... |
| A370-ID01 (a) | 02:39:56.57 | −01:34:26.40 | 25.1 | 1.624 ± 0.065 | 1.925 ± 0.088 | 0.22 ± 0.03 | 1.06 (f) |
| A370-ID02 (a) | 02:39:57.58 | −01:34:53.67 | 9.1 | 1.656 ± 0.182 | 1.778 ± 0.192 | 0.10 ± 0.05 |
 (g) |
| A370-ID03 (a) | 02:39:58.15 | −01:34:24.52 | 7.0 | 0.655 ± 0.094 | 1.007 ± 0.205 | 0.42 ± 0.13 | 1.258 (h) |
| A370-ID04 (b) | 02:39:53.25 | −01:33:29.26 | 4.7 | 0.439 ± 0.094 | ... | ... | ... |
| A370-ID05 (b) | 02:39:53.20 | −01:34:38.16 | 4.5 | 0.283 ± 0.063 | ... | ... | ... |
| AS1063-ID01 (a) | 22:48:49.06 | −44:32:25.39 | 89.3 | 6.295 ± 0.071 | 6.806 ± 0.119 | 0.14 ± 0.01 |
 (g) |
| AS1063-ID02 (a) | 22:48:47.29 | −44:30:48.06 | 10.9 | 1.282 ± 0.118 | 1.273 ± 0.142 | 0.10 ± 0.05 | 1.438 (f) |
| AS1063-ID03 (a) | 22:48:46.58 | −44:30:46.83 | 5.2 | 0.648 ± 0.124 | 1.396 ± 0.399 | 0.45 ± 0.14 |
 (g) |
| AS1063-ID04 (b) | 22:48:41.79 | −44:31:57.80 | 4.9 | 0.338 ± 0.069 | ... | ... | 0.611 (i) |
| AS1063-ID05 (b) | 22:48:42.24 | −44:32:29.20 | 4.6 | 0.320 ± 0.069 | ... | ... | ... |
Notes. Column 1: Source ID. Columns 2, 3: Centroid J2000 position of ID. Column 4: Signal-to-noise ratio of the detection, that is, the ratio of peak intensity and background rms. Column 5: PB-corrected peak intensity and 1σ error. Column 6: PB-corrected integrated flux density and 1σ error from uv fitting. Column 7: Effective radius and 1σ error from uv fitting, defined as 
(half-light radius). Column 8: 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); for sources that lack redshift estimates, we assume a Gaussian redshift distribution with mean z = 2 and σ = 0.5;
spectroscopic redshift from Lagattuta et al. (2022);
The photometric redshift’s best value and 1σ error from SED fitting are presented here only for reference, as we use the full probability distribution found for each photometric redshift.
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