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Table B.1.

Summary of the physical properties derived in this work for our sample, the undetected data set, and GG22.

z bin log M bin Nobj zmedian log M*, median ΔMSmedian log LIR Tdust log Mdust log Mgas, GDR log Mgas, S16 fgas, GDR fgas, S16
(M) (M) (dex) (L) (K) (M) (M) (M)

Whole sample
8≤ log M< 9 910 1.3 8.41 −0.02 10.26 29.36 7.15 10.00 < 0.98
1.0 ≤z< 1.5 9≤ log M< 10 299 1.2 9.37 0.00 10.43 29.36 7.35 9.72 < 0.69
10≤ log M< 11 92 1.2 10.35 0.07 11.18±0.10 30.04 7.97±0.10 10.02±0.30 10.20±0.10 0.32±0.15 0.42±0.05

8≤ log M< 9 1423 1.7 8.41 −0.08 10.21 30.84 6.97 9.97 < 0.97
1.5 ≤z< 2.0 9≤ log M< 10 353 1.8 9.31 0.13 10.66 33.16 7.28 9.80 < 0.75
10≤ log M< 11 96 1.8 10.30 0.17 11.44±0.09 33.49 8.00±0.09 10.14±0.29 10.27±0.09 0.41±0.16 0.48±0.05

8≤ log M< 9 881 2.3 8.50 −0.15 10.38 32.59 7.04 10.12 < 0.98
2.0 ≤z< 2.5 9≤log M< 10 274 2.3 9.31 0.04 10.74 34.70 7.17 9.80 < 0.76
10≤ log M< 11 54 2.2 10.38 −0.03 11.61±0.07 33.59 8.16±0.07 10.34±0.27 10.43±0.07 0.47±0.15 0.53±0.04

8≤ log M< 9 751 2.7 8.56 0.00 10.58 36.21 6.90 10.03 < 0.97
2.5 ≤z≤ 3.0 9≤ log M< 10 340 2.8 9.29 0.06 10.84 37.00 7.12 9.82 < 0.77
10≤ log M< 11 57 2.7 10.32 −0.02 11.71±0.09 36.03 8.04±0.11 10.29±0.31 10.39±0.11 0.48±0.18 0.54±0.06

Undetected data set

1.0 ≤z< 1.5 10≤ log M< 11 85 1.2 10.34 0.06 11.12±0.11 29.93 7.91±0.11 9.97±0.31 10.15±0.11 0.29±0.15 0.39±0.06
1.5 ≤z< 2.0 10≤ log M< 11 84 1.8 10.29 0.12 11.28±0.12 33.01 7.90±0.12 10.05±0.31 10.14±0.12 0.36±0.17 0.42±0.06
2.0 < z≤ 2.5 10≤ log M< 11 46 2.2 10.37 −0.03 11.49±0.10 33.64 8.04±0.10 10.22±0.30 10.30±0.10 0.42±0.17 0.46±0.06
2.5 ≤z≤ 3.0 10≤ log M< 11 47 2.7 10.27 0.00 11.60±0.11 36.17 7.92±0.11 10.19±0.31 10.29±0.11 0.45±0.18 0.51±0.06
G22

1.0 ≤z< 1.5 10≤ log M< 11 4 1.2 10.63 0.10 11.77±0.09 30.33 8.56±0.09 10.55±0.29 10.79±0.09 0.46±0.16 0.59±0.05
1.5 ≤z< 2.0 10≤ log M< 11 9 1.9 10.53 0.34 12.31±0.08 36.02 8.65±0.08 10.74±0.28 10.99±0.08 0.62±0.15 0.74±0.04
2.0 < z≤ 2.5 10≤ log M< 11 6 2.2 10.65 0.09 12.40±0.12 34.77 8.84±0.12 10.94±0.32 11.02±0.12 0.66±0.17 0.70±0.06
2.5 ≤z≤ 3.0 10≤ log M< 11 10 2.8 10.49 0.11 12.26±0.18 37.43 8.51±0.18 10.71±0.37 10.89±0.18 0.62±0.20 0.72±0.09

The Tdust are those corresponding to the Schreiber et al. (2018) templates derived for the galaxies. The subindex GDR denotes that the quantity has been calculated using the gas-to-dust ratio approach. The subindex S16 means that the quantity is derived following Scoville et al. (2016). The lack of uncertainty in the gas fractions, gas and dust masses, and luminosities denotes an upper limit (3σ level). Let us recall that for the undetected data set, we also remove the G13 sources in the neighborhood of the GG22 galaxies. We have three of these neighbor objects at 1 < z < 1.5 and another 3 at 1.5 < z < 2.0 in the high-mass bin; 2 at 2.0 < z < 2.5, and none at 2.5 < z < 3.0.

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