Table A.1.
Summary of fluxes (peak flux using Blobcat and integrated flux using uvmodelfit), as well as the sizes (measured using uvmodelfit) for the galaxies in the Main and Supplementary catalogs.
| ID |
 |
 |
FHWMuvmodelfit |
|---|---|---|---|
| (mJy) | (mJy) | (arcsec) | |
| AGS1 | 1.90 ± 0.20* | 2.20 ± 0.13 | 0.21 ± 0.02 |
| AGS2 | 1.99 ± 0.22* | 2.31 ± 0.12 | 0.16 ± 0.01 |
| AGS3 | 1.84 ± 0.21* | 1.97 ± 0.12 | 0.16 ± 0.16 |
| AGS4 | 1.72 ± 0.20* | 1.68 ± 0.11 | 0.18 ± 0.02 |
| AGS5 | 1.56 ± 0.19* | 2.49 ± 0.18 | 0.19 ± 0.02 |
| AGS6 | 1.27 ± 0.18* | 1.37 ± 0.13 | 0.11 ± 0.03 |
| AGS7 | 1.15 ± 0.17* | 1.64 ± 0.11 | 0.10 ± 0.02 |
| AGS8 | 1.43 ± 0.22* | 2.23 ± 0.17 | 0.23 ± 0.02 |
| AGS9 | 1.25 ± 0.21* | 1.70 ± 0.18 | 0.23 ± 0.03 |
| AGS10 | 0.88 ± 0.15* | 1.18 ± 0.13 | 0.14 ± 0.03 |
| AGS11 | 1.34 ± 0.25* | 1.71 ± 0.17 | 0.12 ± 0.02 |
| AGS12 | 0.93 ± 0.18* | 1.17 ± 0.15 | 0.22 ± 0.04 |
| AGS13 | 0.78 ± 0.15* | 0.84 ± 0.11 | 0.17 ± 0.03 |
| AGS15 | 0.80 ± 0.16 | 1.21 ± 0.11* | 0.07 ± 0.02 |
| AGS17 | 0.93 ± 0.19 | 2.30 ± 0.20* | 0.41 ± 0.03 |
| AGS18 | 0.85 ± 0.18 | 1.70 ± 0.28* | 0.50 ± 0.08 |
| AGS20 | 1.11 ± 0.24* | 1.90 ± 0.20 | 0.19 ± 0.02 |
| AGS21 | 0.64 ± 0.11* | 0.75 ± 0.12 | 0.09 ± 0.04 |
| AGS23 | 0.98 ± 0.21* | 0.94 ± 0.16 | 0.22 ± 0.04 |
| AGS24 | 0.88 ± 0.22* | 0.81 ± 0.29 | 0.06 ± 0.55 |
| AGS25 | 0.81 ± 0.19* | 1.06 ± 0.28 | 0.12 ± 0.24 |
| AGS26 | 0.74 ± 0.18 | 0.97 ± 0.15* | 0.30 ± 0.09 |
| AGS27 | 0.82 ± 0.22 | 1.43 ± 0.28* | 0.54 ± 0.12 |
| AGS28 | 0.85 ± 0.21 | 1.56 ± 0.21* | 0.50 ± 0.07 |
| AGS29 | 0.61 ± 0.18* | 1.22 ± 0.19 | ... |
| AGS30 | 0.67 ± 0.17* | 0.83 ± 0.23 | ... |
| AGS31 | 0.72 ± 0.19* | 1.01 ± 0.17 | ... |
| AGS32 | 0.63 ± 0.16 | 1.23 ± 0.16* | 0.33 ± 0.10 |
| AGS33 | 0.70 ± 0.19 | 1.77 ± 0.27* | 0.51 ± 0.10 |
| AGS34 | 0.55 ± 0.15* | ... | ... |
| AGS35 | 0.65 ± 0.18 | 1.16 ± 0.21* | 0.45 ± 0.12 |
| AGS36 | 0.74 ± 0.21* | 0.74 ± 0.18 | 0.23 ± 0.13 |
| AGS37 | 0.63 ± 0.18 | 1.10 ± 0.16* | 0.28 ± 0.10 |
| AGS38 | 0.58 ± 0.16 | 1.00 ± 0.16* | 0.32 ± 0.10 |
| AGS39 | 0.80 ± 0.23* | 0.98 ± 0.28 | 0.25 ± 0.14 |
Notes. For each galaxy, the flux used (as explained in F18 and F20a) is indicated by an asterisk. The absence of a size indicates a nonconvergence of uvmodelfit. For AGS15, we obtained new 2 mm ALMA data for this galaxy, (project 2018.1.01079.S PI: M. Franco; see Zhou et al. 2020), which led us to revise our hypothesis that the source was compact and to favor the uvmodelfit flux which is in agreement with the 2 mm flux and the flux at 850 μm (Cowie et al. 2018).
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