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Table 7
Input parameters used to fit the HRS galaxies.
| Parameter | Value | Units |
|
|
||
| Pop. synth. mod. | Bruzual & Charlot (2003) | |
| Dust model | Draine & Li (2007) | |
| IMF | Salpeter | |
| Metallicity | 0.02 | |
| Velocity | 40–360 in step of 10 | km s-1 |
| QF | –0.4, –0.2, 0.2, 0.4, 0.6, 0.7, 0.8, 0.9, 0.95, 1 | |
| QA | 0, 5, 10, 20, 50, 100, 150, 200, 250, 300, 400, 500, 600, 700, 800, 900, 1000, 1250, 1500, 2000, 3000 | Myr |
| E(B−V)young | 0.05, 0.1, 0.2, 0.4 | |
| E(B−V)old | 0.44 | |
| Q PAH | 0.47, 2.50, 4.58, 6.63, 7.32 | |
| U min | 0.1, 0.5, 2.0, 4.0, 8.0, 20 | |
| α | 2.0, 2.5, 3.0 | |
| γ | 0.01, 0.03, 0.1 | |
Notes. The input parameters used in the analysis of the HRS span a wider range than those used to create the mock galaxies to avoid border effects.
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