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Home All issues Volume 659 (March 2022) A&A, 659 (2022) A196 Full HTML
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Table 1.

Dust and stellar-based properties.

ID z log(M*/M⊙) log(LIR/L⊙) SFR ΔMS log(Mdust/M⊙) Tdust log(Mgas/M⊙) fgas τdep
(M⊙ yr−1) (K) (Myr)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
A2GS1 2.309 11.06 12.80 ± 0.01 1093 ± 10 5.59 ± 0.05 9.03 ± 0.01 42.4 11.09 ± 0.20 0.52 ± 0.11 112 ± 51
A2GS2 3.556 11.09 12.92 ± 0.01 1428 ± 31 3.79 ± 0.08 8.93 ± 0.01 45.0 11.07 ± 0.20 0.49 ± 0.11 82 ± 37
A2GS3( † ) 2.582 11.44 12.86 ± 0.01 1251 ± 13 2.96 ± 0.03 9.03 ± 0.01 44.1 11.03 ± 0.20 0.28 ± 0.09 85 ± 39
A2GS4 2.918 10.76 12.92 ± 0.01 1416 ± 24 10.03 ± 0.17 8.97 ± 0.01 46.0 11.17 ± 0.20 0.72 ± 0.09 103 ± 47
A2GS5 1.797 11.09 12.55 ± 0.01 614 ± 11 4.37 ± 0.08 9.44 ± 0.01 32.8 11.45 ± 0.20 0.70 ± 0.10 460 ± 210
A2GS6 3.46 11.14 12.88 ± 0.01 1312 ± 29 3.25 ± 0.07 8.93 ± 0.01 45.6 11.05 ± 0.20 0.45 ± 0.11 85 ± 39
A2GS7 3.467 10.52 13.00 ± 0.03 1750 ± 100 17.7 ± 1.0 8.95 ± 0.03 (…) 11.28 ± 0.20 0.85 ± 0.06 108 ± 50
A2GS8( * ) 3.29 11.44 12.59 ± 0.04 665 ± 57 1.02 ± 0.09 8.91 ± 0.04 (…) 10.95 ± 0.20 0.24 ± 0.09 133 ± 63
A2GS9 2.696 10.90 12.30 ± 0.03 345 ± 22 1.95 ± 0.12 8.92 ± 0.03 31.3 11.06 ± 0.20 0.59 ± 0.11 330 ± 150
A2GS10( * ) 3.47 10.56 12.91 ± 0.03 1415 ± 85 13.03 ± 0.78 8.86 ± 0.03 (…) 11.18 ± 0.20 0.80 ± 0.07 106 ± 49
A2GS11( † ) 2.41 11.33 12.61 ± 0.01 694 ± 13 2.16 ± 0.04 9.05 ± 0.01 39.7 11.06 ± 0.20 0.35 ± 0.10 165 ± 76
A2GS12 3.847 10.87 12.62 ± 0.03 724 ± 52 2.89 ± 0.21 8.83 ± 0.03 (…) 11.05 ± 0.20 0.60 ± 0.11 156 ± 73
A2GS13 1.619 10.96 12.48 ± 0.01 521 ± 3 5.27 ± 0.03 9.18 ± 0.01 34.4 11.19 ± 0.20 0.63 ± 0.11 300 ± 140
A2GS14 1.956 11.19 12.32 ± 0.01 361 ± 4 1.95 ± 0.02 8.97 ± 0.01 36.3 10.97 ± 0.20 0.38 ± 0.11 260 ± 120
A2GS15 3.47 10.24 12.36 ± 0.02 391 ± 22 7.53 ± 0.42 8.81 ± 0.02 39.2 11.25 ± 0.20 0.91 ± 0.04 460 ± 210
A2GS16( † ) 2.45 11.39 12.33 ± 0.03 364 ± 21 1.01 ± 0.06 8.69 ± 0.03 40.7 10.69 ± 0.20 0.17 ± 0.06 130 ± 62
A2GS17( * ) 4.64 10.39 12.84 ± 0.04 1200 ± 110 11.5 ± 1.1 8.54 ± 0.04 (…) 11.00 ± 0.20 0.80 ± 0.07 84 ± 40
A2GS18( * ) 3.689 10.56 12.63 ± 0.05 738 ± 79 6.33 ± 0.68 8.52 ± 0.05 (…) 10.85 ± 0.20 0.66 ± 0.10 96 ± 46
A2GS19( † ) 2.225 11.43 12.39 ± 0.01 427 ± 10 1.35 ± 0.03 8.60 ± 0.01 43.4 10.57 ± 0.20 0.12 ± 0.05 85 ± 39
A2GS20 2.68 10.72 11.96 ± 0.04 157 ± 13 1.34 ± 0.11 9.20 ± 0.04 (…) 11.39 ± 0.20 0.82 ± 0.07 1540 ± 730
A2GS21 2.698 10.30 12.57 ± 0.01 639 ± 19 14.24 ± 0.43 8.89 ± 0.01 37.1 11.22 ± 0.20 0.90 ± 0.04 260 ± 120
A2GS22 2.72 10.77 12.22 ± 0.02 286 ± 14 2.14 ± 0.11 8.90 ± 0.02 35.4 11.07 ± 0.20 0.67 ± 0.10 410 ± 190
A2GS23 2.00 10.76 12.25 ± 0.01 306 ± 8 3.33 ± 0.09 8.97 ± 0.01 35.3 11.08 ± 0.20 0.67 ± 0.10 390 ± 180
A2GS24 2.32 11.38 12.33 ± 0.01 364 ± 12 1.13 ± 0.04 9.13 ± 0.01 36.0 11.12 ± 0.20 0.35 ± 0.10 360 ± 160
A2GS25 2.543 10.13 12.81 ± 0.01 1099 ± 11 38.65 ± 0.39 8.82 ± 0.01 48.9 11.21 ± 0.20 0.92 ± 0.03 145 ± 66
A2GS26 1.927 10.64 11.55 ± 0.04 61 ± 6 0.89 ± 0.09 9.22 ± 0.04 (…) 11.36 ± 0.20 0.84 ± 0.06 3700 ± 1800
A2GS27( * ) 4.72 11.01 12.39 ± 0.08 426 ± 77 0.96 ± 0.17 8.39 ± 0.08 (…) 10.61 ± 0.21 0.29 ± 0.10 96 ± 50
A2GS28 1.967 10.71 12.22 ± 0.02 283 ± 10 3.48 ± 0.12 8.60 ± 0.02 38.1 10.72 ± 0.20 0.50 ± 0.11 183 ± 84
A2GS29( * ) 3.47 11.32 12.40 ± 0.05 436 ± 54 0.75 ± 0.09 8.69 ± 0.05 (…) 10.76 ± 0.21 0.22 ± 0.08 131 ± 64
A2GS30( † ) 3.80 11.46 12.81 ± 0.01 1099 ± 37 1.28 ± 0.04 8.75 ± 0.01 59.1 10.81 ± 0.20 0.18 ± 0.07 58 ± 27
A2GS31( † ) 2.15 11.18 12.27 ± 0.01 322 ± 8 1.51 ± 0.04 8.77 ± 0.01 38.1 10.79 ± 0.20 0.29 ± 0.09 188 ± 86
A2GS32( † ) 2.251 11.55 12.39 ± 0.02 426 ± 20 1.15 ± 0.05 8.95 ± 0.02 36.8 10.90 ± 0.20 0.18 ± 0.07 188 ± 86
A2GS33( * ) (…) (…) (…) (…) (…) (…) (…) (…) (…) (…)
A2GS34( † ) 1.613 11.43 12.00 ± 0.01 170 ± 4 0.98 ± 0.02 8.84 ± 0.01 33.0 10.78 ± 0.20 0.18 ± 0.07 350 ± 160
A2GS35( † ) 4.73 10.94 12.77 ± 0.02 1001 ± 41 2.65 ± 0.11 8.23 ± 0.02 (…) 10.48 ± 0.20 0.26 ± 0.09 30 ± 14
A2GS36( † ) 2.36 11.27 12.06 ± 0.02 196 ± 10 0.69 ± 0.03 8.52 ± 0.02 34.5 10.54 ± 0.20 0.16 ± 0.06 175 ± 81
A2GS37( * ) 3.85 11.16 12.33 ± 0.07 372 ± 63 0.76 ± 0.13 8.54 ± 0.07 (…) 10.67 ± 0.21 0.25 ± 0.09 126 ± 65
A2GS38( * ) (…) (…) (…) (…) (…) (…) (…) (…) (…) (…)
A2GS39 2.36 10.61 12.44 ± 0.01 478 ± 7 6.02 ± 0.09 8.77 ± 0.01 40.9 10.96 ± 0.20 0.69 ± 0.10 192 ± 88
A2GS40( * ) 2.46 10.21 12.40 ± 0.09 432 ± 86 13.1 ± 2.6 8.57 ± 0.09 (…) 10.92 ± 0.22 0.84 ± 0.07 192 ± 100
A2GS41 1.759 10.54 11.88 ± 0.01 129 ± 4 2.58 ± 0.08 9.06 ± 0.01 28.3 11.20 ± 0.20 0.82 ± 0.07 1220 ± 560
A2GS42( † ) 2.29 11.12 12.13 ± 0.02 233 ± 9 1.09 ± 0.04 8.80 ± 0.02 34.9 10.84 ± 0.20 0.35 ± 0.10 300 ± 140
A2GS43 3.54 10.54 12.88 ± 0.02 1319 ± 52 12.45 ± 0.49 8.53 ± 0.02 65.8 10.85 ± 0.20 0.67 ± 0.10 54 ± 25
A2GS44( † ) 4.19 11.05 12.71 ± 0.02 888 ± 34 2.12 ± 0.08 8.56 ± 0.02 (…) 10.74 ± 0.20 0.33 ± 0.10 62 ± 28

Notes. A2GS1 to A2GS44 correspond to the 100% pure source catalog in Gómez-Guijarro et al. (2022). (1) ALMA source ID with galaxies without a Herschel counterpart followed by (*); (2) redshift with spectroscopic redshifts shown with three decimal digits (see Gómez-Guijarro et al. 2022 for the spectroscopic redshift references therein); (3) stellar mass; (4) IR luminosity (8−1000 μm rest-frame) as obtained from Stardust for the galaxies with a Herschel counterpart accounting for star formation only (without AGN contribution) or from the iterative approach using the dust SED libraries by Schreiber et al. (2018) for the galaxies without a Herschel counterpart (see Sect. 3.2); (5) total SFR accounting for the contribution of the obscured star formation probed in the IR (SFRIR) and the unobscured star formation probed in the UV (SFRUV); (6) distance to the MS (where the MS is from Schreiber et al. 2015) defined as the ratio of the SFR to the SFR of the MS at the same stellar mass and redshift (ΔMS = SFR/SFRMS); (7) dust mass as obtained from Stardust for the galaxies with a Herschel counterpart or from the iterative approach using the dust SED libraries by Schreiber et al. (2018) for the galaxies without a Herschel counterpart (see Sect. 3.2); (8) dust temperature obtained from a MBB fit for the galaxies with a Herschel counterpart (see Sect. 3.5); (9) gas mass as obtained from the metallicity-dependent gas-to-dust mass ratio technique (see Sect. 3.4); (10) gas fraction (fgas = Mgas/(Mgas + M*)); (11) depletion timescale (τdep = Mgas/SFR) (see Sect. 3.4). A2GS33 and A2GS38 lack any estimate as these are Ks dropouts (A2GS33 a candidate Spitzer/IRAC 3.6 μm dropout) and, thus, they lack of robust redshift and stellar mass estimates to attempt an IR SED fitting and to derive dust and stellar-based properties (see Gómez-Guijarro et al. 2022). We note that among the galaxies with a Herschel counterpart there are two galaxies for which the mid-IR to mm photometry is not satisfactory and we treated them following the iterative approach with the dust SED libraries by Schreiber et al. (2018) (namely A2GS7 and A2GS12). Besides, some of the galaxies lack a Tdust estimate as they did not meet the MBB fitting criteria or the mid-IR to millimeter photometry was scarce and the fit did not converge (see Sect. 3.5). Galaxies classified as SBs in the MS following the definition in Sect. 4 are highlighted with (†).

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