Table A.1.
Characteristics of the ALMA Band 8 observations analyzed in this work.
| ID | N. ant. | Beam size | Rms | S(407 GHz) |
|---|---|---|---|---|
| (arcsec) | (mJy/beam) | (mJy) | ||
| AJ025-33 | 11-13 | 1.96 × 1.62 | 0.16 | 6.8 ± 0.7 |
| J0305-3150 | 8 | 4.44 × 2.75 | 0.95 | 10.4 ± 1.5 |
| J0439+1634* | 14 | 2.53 × 1.38 | 1.0 | 45.4 ± 4.7 |
| J2318-3029 | 10 | 3.96 × 2.62 | 0.65 | 6.9 ± 1.0 |
| J2348–3054 | 8 | 4.31 × 2.59 | 0.44 | 5.5 ± 0.7 |
| PJ007+04 | 15 | 1.91 × 1.51 | 0.19 | 4.8 ± 0.6 |
| PJ009–10 | 8 | 4.14 × 2.65 | 0.80 | 8.6 ± 1.2 |
| PJ036+03 | 14 | 1.92 × 1.46 | 0.24 | 6.2 ± 0.7 |
| PJ083+11 | 13 | 2.91 × 1.35 | 0.58 | 10.5 ± 1.5 |
| PJ158-14 | 12 | 1.80 × 1.49 | 0.45 | 9.6 ± 1.2 |
| PJ231–20** | 10 | 4.34 × 2.92 | 0.92 | 9.6 ± 1.6 |
Notes. Columns: QSO name; number of antennas; clean beam size; root mean squared of the noise in the clean continuum map; measured flux at the observed frequency of 407 GHz. A 10% systematic flux calibration uncertainty was added in quadrature to the nominal uncertainty. *this source is strongly lensed, **this source has an unresolved companion.
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