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Parameter | Description | Fiducial value | Source of constraints |
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Inverse of star formation efficiency | 50 | Kennicutt (1998) |
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Inverse of mass loading for feedback | 0.1 | Martin et al. (2002) |
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Galaxy merger power law | 3.333 | Numerical simulations e.g. Walker et al. (1996) |
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Baryon fraction | 0.02 h-2 | 2H abundance in QSO absorption lines (Tytler et al. 1996) |
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S-S merging normalisation | 0.017 | Makino & Hut (1997) |
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Recycling efficiency | 0.3 | Set to fiducial value in Hatton et al. (2003) |
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Ratio of burst-to-bulge radius | 0.1 | Set to fiducial value in Hatton et al. (2003) |
Dust | ISM Extinction and emission due to dust | - | Guiderdoni et al. (1987), Desert et al. (1990) |
IMF | Initial mass function | - | Kennicutt (1983) |
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