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Table B.1
Dusty star-forming galaxies evolution model parameters, fitted to selected infrared observations.
| Parameter | Description | Value |
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| α | Faint-end slope of the infrared bolometric LF | 1.223 ± 0.044 |
| σ | Parameter driving the bright-end slope of the LF | 0.406 ± 0.019 |
| L⋆(z = 0) ( × 1010 L⊙) | Local characteristic luminosity of the LF | 2.377 ± 0.363 |
| φ⋆ (z = 0) ( × 10-3 gal/dex/Mpc3) | Local characteristic density of the LF | 3.234 ± 0.266 |
| rL⋆,lz | Evolution of the characteristic luminosity between 0 and zbreak,1 | 2.931 ± 0.119 |
| r phi⋆,lz | Evolution of the characteristic density between 0 and zbreak,1 | 0.774 ± 0.196 |
| zbreak,1 | Redshift of the first break | 0.879 ± 0.052 |
| rL⋆ ,mz | Evolution of the characteristic luminosity between zbreak,1 and zbreak,2 | 4.737 ± 0.301 |
| r phi⋆,mz | Evolution of the characteristic density of between zbreak,1 and zbreak,2 | -6.246 ± 0.458 |
| z break,2 | Redshift of the second break | 2.000(fixed) |
| rL⋆,hz | Evolution of the characteristic luminosity for z > zbreak,2 | 0.145 ± 0.460 |
| rphi⋆,hz | Evolution of the characteristic density for z > zbreak,2 | -0.919 ± 0.651 |
| Lpop ( × 1010 L⊙) | Luminosity of the transition between normal and starburst templates | 23.677 ± 2.704 |
| σpop | Width of the transition between normal and starburst templates | 0.572 ± 0.056 |
Notes. Table extracted from Béthermin et al. 2011. The errors are derived from a MCMC analysis.
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