Table 3
Integrated properties of the ALMA sources.
| ID | S | LIR | SFRtot | SFRSED | log10 (M⋆) | RSB | log10(LX) |  |
 |
τdep |
|---|---|---|---|---|---|---|---|---|---|---|
| M | (× 1011L⊙) | (M⊙ yr−1) | (M⊙ yr−1) | (M⊙) | (erg.s−1) | (× 108M⊙) | (× 1010M⊙) | (Myr) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| GS1 | S | 17.6 ± 0.9 | 306 ± 15 | 107 | 11.18 | 1.39 | 43.44 | 4.2 ± 0.4 | 4.9 ± 0.5 | 161 ± 24 |
| GS2 | S | 22.2 ± 1.9 | 385 ± 32 | 100 | 11.23 | 1.47 | – | 5.1 ± 0.5 | 6.0 ± 0.6 | 156 ± 28 |
| GS3 | S | 25.3 ± 1.3 | 438 ± 22 | 112 | 11.28 | 1.66 | 43.44 | 5.5 ± 0.3 | 6.3 ± 0.3 | 144 ± 14 |
| GS4 | S | 20.9 ± 1.8 | 360 ± 31 | 290 | 11.29 | 1.70 | – | 8.2 ± 1.1 | 9.3 ± 1.3 | 258 ± 57 |
| GS5 | S | 66.8 ± 3.3 | 1154 ± 57 | 339 | 11.54 | 2.41 | 43.54 | 14.5 ± 0.7 | 15.1 ± 0.8 | 131 ± 13 |
| GS6 | M | 66.1 ± 3.3 | 1139 ± 57 | 107 | 11.28 | 4.10 | 42.29 | 15.7 ± 1.2 | 17.9 ± 1.4 | 158 ± 20 |
| GS7 | M | 27.9 ± 1.4 | 482 ± 24 | 241 | 10.90 | 5.36 | 42.05 | 10.1 ± 1.2 | 13.8 ± 1.6 | 286 ± 48 |
| GS8 | U | 58.8 ± 3.6 | 1016 ± 61 | 567 | 11.49 | 1.49 | 43.26 | 21.3 ± 4.1 | 22.4 ± 4.3 | 220 ± 55 |
| UDF1 | U | 57.4 ± 2.9 | 987 ± 49 | 536 | 11.03 | 3.45 | 43.92 | 12.6 ± 0.8 | 16.0 ± 1.0 | 162 ± 18 |
| UDF2 | M | 26.0 ± 1.3 | 448 ± 22 | 120 | 11.07 | 1.71 | – | 8.3 ± 1.1 | 10.3 ± 1.4 | 231 ± 42 |
| UDF3 | M | 53.4 ± 2.7 | 928 ± 46 | 41 | 10.13 | 32.61 | 42.66 | 11.3 ± 0.6 | 25.4 ± 1.3 | 274 ± 27 |
| UDF4 | M | 10.6 ± 0.6 | 183 ± 11 | 48 | 10.60 | 2.17 | – | 2.9 ± 0.3 | 4.7 ± 0.5 | 257 ± 43 |
| UDF5 | M | 7.7 ± 0.4 | 132 ± 7 | 127 | 10.39 | 3.67 | – | 4.8 ± 0.8 | 8.8 ± 1.5 | 669 ± 147 |
| UDF6 | S | 9.1 ± 0.5 | 157 ± 8 | – | 10.71 | 2.88 | – | 4.0 ± 0.6 | 6.0 ± 0.9 | 383 ± 76 |
| UDF7 | M | 11.2 ± 0.6 | 194 ± 10 | 95 | 10.49 | 2.93 | 42.68 | 2.5 ± 0.2 | 4.4 ± 0.3 | 224 ± 26 |
| UDF8 | S | 9.9 ± 0.5 | 173 ± 9 | 154 | 11.12 | 1.49 | 43.70 | 3.2 ± 0.5 | 3.9 ± 0.6 | 227 ± 44 |
| UDF11 | M | 22.5 ± 1.1 | 396 ± 19 | 267 | 10.80 | 3.99 | 42.38 | 4.8 ± 0.2 | 6.9 ± 0.3 | 173 ± 17 |
| UDF13 | S | 7.4 ± 0.5 | 128 ± 9 | 166 | 10.81 | 0.96 | 42.45 | 1.9 ± 0.3 | 2.7 ± 0.4 | 214 ± 46 |
| UDF16 | S | 3.2 ± 0.2 | 54 ± 3 | – | 10.80 | 1.01 | – | 1.7 ± 0.5 | 2.4 ± 0.7 | 439 ± 145 |
Notes: Column (1) simplified ID. Column (2) visual morphological classification of the rest-frame optical images of the galaxies (from HST-WFC3 H-band): single/isolated galaxy (S), merger (M) and undefined (U). Column (3) total IR (8–1000 μm) luminosity measured from the fit of the data from Spitzer, Herschel, and ALMA. Column (4) total SFR = SFRIR+SFRUV in M⊙ yr−1 where both SFR are defined in Eqs. (5) and (6). Column (5)SFR derived from the fit of the UV-optical-NIR SED in M⊙ yr−1 assuming a contant SFR history. Column (6) logarithm of the stellar mass (Salpeter IMF). Column (7) starburstiness, RSB = SFR/SFRMS, where SFRMS is the MS SFR at the redshift of the galaxy. Column (8) logarithm of the total 0.5–8 keV X-ray luminosities in erg s−1 from Luo et al. (2017). Column (9) dust mass derived from the fit of the FIR SED (see Sect. 2.4). Column (10) gas mass derived from the dust mass in Column (9) following the recipe for the dust-to-gas ratio described in Sect. 2.4. Column (11) depletion time, τdep (= Mgas/SFR), in Myr.
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