Table 3.
Main physical properties of the sample of 42 453 galaxies presented in total IR luminosity bins.
| Ngal | NAGN | Redshift | log(Mstar) | log(SFR) | log(sSFR) | |
|---|---|---|---|---|---|---|
| (%) | (%) | (M⊙ | (M⊙ yr−1) | (yr−1) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| log(Ldust) < 11 | 6974 | 268 | 0.42 ± 0.15 | 10.12 ± 0.34 | 0.64 ± 0.27 | −9.70 ± 0.16 |
| 16.43% | 3.86% | |||||
| LIRGs 11 ≤ log(Ldust) < 12 | 23 214 | 724 | 0.96 ± 0.27 | 10.73 ± 0.24 | 1.59 ± 0.23 | −9.22 ± 0.31 |
| 54.68% | 3.11% | |||||
| ULIRGs 12 ≤ log(Ldust) < 13 | 11 947 | 705 | 1.89 ± 0.32 | 11.10 ± 0.22 | 2.30 ± 0.17 | −8.85 ± 0.21 |
| 28.14% | 5.90% | |||||
| HLIRGs log(Ldust) ≽ 13 | 318 | 65 | 4.92 ± 0.34 | 11.49 ± 0.34 | 3.52 ± 0.17 | −8.01 ± 0.53 |
| 0.75% | 20.44% |
Notes. The first column corresponds to the galaxy type according to their total log(Ldust) value, the second shows the number of galaxies (first row), and the total percentage of the sample (second row), Col. (3) presents the number of galaxies with an AGN contribution higher than 20% (first row – total number, second row – percentage value of galaxiwhiches with AGN contribution within the given IR luminosity bin). Median values for redshift, stellar mass, SFR and specific SFR are given in Cols. (4)–(7). The errors are calculated as median absolute deviation.
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