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Table 1
Parameters of our model.
| Parameter name | Description | Value |
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| Mmin | Minimal mass for a halo to have a central galaxy | 1011.5 M⊙ |
| Msat | Nomalization mass for satellite galaxies | 1012.5 M⊙ |
| αsat | Slope of the number of satellite galaxies at high mass | 1.4 |
| σlog M | Scatter in halo mass | 0.65 |
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| α | Faint end slope of the IR bolometric LF | 1.223 |
| σ | Parameter driving the bright end slope | 0.406 |
| L⋆(z = 0) | Local characteristic luminosity of the LF | 2.377 × 1010 L⊙ |
| φ⋆(z = 0) | Local characteristic density of the LF | 3.234 × 10-3 gal/dex/Mpc3 |
| rL⋆, lz | Evolution of the characteristic luminosity between 0 and zbreak | 2.931 |
| rφ⋆, lz | Evolution of the characteristic density between 0 and zbreak | 0.774 |
| zbreak | Redshift of the first break | 0.879 |
| rL⋆ ,mz | Evolution of the characteristic luminosity between zbreak and 2 | 4.737 |
| rφ ⋆ ,mz | Evolution of the characteristic density between zbreak and 2 | −6.246 |
| rL ⋆ ,hz | Evolution of the characteristic luminosity for z > 2 | 0.145 |
| rφ ⋆ ,hz | Evolution of the characteristic density for z > 2 | −0.919 |
| Lpop | Luminosity of the transition between normal and star-forming templates | 23.677 × 1010 |
| σpop | Width of the transition between normal and star-forming templates | 0.57 |
Notes. The first part of the table lists the halo model parameters and the second part lists the parameters of the model of galaxies. The values of the latter are the mean ones of Béthermin et al. (2011).
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