Table 1.
Properties of the A3COSMOS and A3GOODSS databases.
| Database | COSMOS | GOODS-S |
|---|---|---|
| ALMA projects | 173 | 74 |
| Continuum images | 3232 | 723 |
| Blind survey images | 14 | 49 |
| Spatial coverage [arcmin2] | ||
| Band 3 | 427.7 (205.6) | 101.0 (77.4) |
| Band 4 | 224.8 (205.2) | 44.5 (21.2) |
| Band 5 | 2.6 (1.1) | 1.9 (1.0) |
| Band 6 | 289.3 (127.9) | 90.7 (86.8) |
| Band 7 | 183.3 (81.0) | 38.5 (17.8) |
| Band 8 | 3.3 (1.4) | 0.1 (0.05) |
| Band 9 | 0.08 (0.04) | 0.5 (0.2) |
| Combined | 896.3 (519.6) | 149.6 (115.9) |
| Photometry catalogues | ||
| Blind catalogue | 2204 | 491 |
| Prior catalogue | 2540 | 568 |
| Unique sources | ||
| Total | 1756 | 294 |
| Blind-only | 131 | 79 |
| With prior photometry | 1625 | 215 |
| With prior redshift | 1514 | 185 |
| SED outliers | 86 | 37 |
| CPA discarded | 117 | 60 |
| Robust Galaxy Catalogue | 1335 | 127 |
Notes. Listed by field are the number of ALMA projects, pipeline-produced continuum images, and blind surveys; spatial coverage (taking overlapping areas into account) per ALMA band considering the area where the primary beam attenuation is > 0.2 (in brackets: > 0.5, as displayed in Fig. 1); number of valid detections in the blind (S/Npeak > 5.4) and prior (S/Npeak > 4.35) catalogues; number of unique sources with prior photometry available and with prior photometric or spectroscopic redshift information (both required for SED fitting), sources discarded due to disagreement with the SED fit (SED outliers), sources discarded due to unreliable counterpart association (CPA discarded), and final number of sources in our Robust Galaxy Catalogue including galaxy properties inferred from SED fitting.
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