Table 3
Evolution of dust attenuation at UV wavelength with redshift for the fiducial model (B12 attenuation curve and AGN 2) and galaxies with a luminosity close to 
.
| Bin | N | ⟨ z ⟩ | ⟨ log (LIR) ⟩ | ⟨ log (Mstar) ⟩ | ⟨ AUV ⟩ |
| L ⊙ | M ⊙ | mag | |||
|
|
|||||
| 1 | 795 | 0.4 | 10.78 | 10.41 | 3.32 |
| 2−1 | 479 | 0.9 | 11.46 | 10.61 | 4.20 |
| 2.2 | 726 | 1.2 | 11.68 | 10.73 | 4.04 |
| 3 | 282 | 1.5 | 11.96 | 10.96 | 3.93 |
Notes. Mean values of redshift, LIR, Mstar, and AUV as well as the number N of sources used are reported for each redshift bin (bin 2 is split in two subbins, see text). The dispersion of AUV is on the order of 1.3 mag in each bin (as plotted in Fig. 10).
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