Table A.1.
Mdust estimates for the 23 ALPINE continuum detected sources.
| Target Name | log Mdust |
|---|---|
| [log10(M/M⊙)] | |
| CANDELS_GOODSS_19 | 8.21±0.19 |
| CANDELS_GOODSS_32 | 8.12± 0.21 |
| DEIMOS_COSMOS_396844 | 8.31± 0.19 |
| DEIMOS_COSMOS_417567 | 8.22± 0.21 |
| DEIMOS_COSMOS_422677 | 8.33± 0.22 |
| DEIMOS_COSMOS_460378 | 7.95± 0.21 |
| DEIMOS_COSMOS_488399 | 8.32 ± 0.18 |
| DEIMOS_COSMOS_493583 | 8.14 ± 0.22 |
| DEIMOS_COSMOS_494057 | 8.16 ± 0.18 |
| DEIMOS_COSMOS_539609 | 8.13 ± 0.21 |
| DEIMOS_COSMOS_552206 | 8.35 ± 0.20 |
| DEIMOS_COSMOS_683613 | 8.29± 0.19 |
| DEIMOS_COSMOS_818760 | 8.81± 0.17 |
| DEIMOS_COSMOS_848185 | 8.38± 0.18 |
| DEIMOS_COSMOS_873756 | 8.91± 0.17 |
| DEIMOS_COSMOS_881725 | 8.32±0.25 (a) |
| vuds_cosmos_5100822662 | 8.09± 0.18 |
| vuds_cosmos_5100969402 | 8.29± 0.21 |
| vuds_cosmos_5100994794 | 7.85± 0.21 |
| vuds_cosmos_5101209780 | 8.27± 0.23 (a) |
| vuds_cosmos_5101218326 | 8.44± 0.18 |
| vuds_cosmos_5180966608 | 8.39± 0.19 |
| vuds_efdcs_530029038 | 7.85± 0.26 (a) |
Notes. The dust masses were estimated using a modified black-body (MBB) spectrum, under the approximation of thin emission, assuming Tdust = 25 K and the spectral index β = 1.8 (see Sect. 3). (a)Multi-component objects (see Appendix D.2 and Table D.1 in Béthermin et al. 2020). For DEIMOS_COSMOS_881725 the sum of the components was considered; for vuds_cosmos_51012097 and vuds_efdcs_530029038 only the fluxes of the central targets were considered since the companions are likely separated objects (see Sect. 2).
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