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Table 2.
Best-fit parameters at the knee of the IR-LF.
| z | log(L*/L⊙) | log(L*/L⊙) | log(L*/L⊙) | log(Φ∗/Mpc−3 dex−1) | log(Φ∗/Mpc−3 dex−1) | log(Φ∗/Mpc−3 dex−1) |
|---|---|---|---|---|---|---|
| 16th | 50th | 84th | 16th | 50th | 84th | |
| 0.5 − 1.0 | 10.93 | 10.94 | 10.95 | −2.49 | −2.44 | −2.40 |
| 1.0 − 1.5 | 11.27 | 11.29 | 11.31 | −2.84 | −2.77 | −2.73 |
| 1.5 − 2.0 | 11.58 | 11.61 | 11.66 | −3.19 | −3.09 | −3.04 |
| 2.0 − 2.5 | 11.79 | 11.84 | 11.90 | −3.44 | −3.32 | −3.24 |
| 2.5 − 3.0 | 11.93 | 12.05 | 12.15 | −3.71 | −3.55 | −3.46 |
| 3.0 − 3.5 | 11.93 | 12.07 | 12.27 | −3.90 | −3.71 | −3.61 |
| 3.5 − 4.5 | 11.81 | 12.05 | 12.47 | −4.20 | −3.97 | −3.84 |
| 4.5 − 6.0 | 11.57 | 12.07 | 12.69 | −4.53 | −4.24 | −4.10 |
Notes. Luminosities (L*) and normalizations (Φ*) with 16th, 50th, and 84th percentiles at the knee in the eight redshift bins obtained through the MCMC analysis or, in the ALMA+Herschel case, using the information from all the redshifts together.
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