Table C.1.
Modules and their corresponding parameters used for this work to build a grid of 289 536 models per redshift for every set of stellar population models.
| Module | Parameter | Value | |
|---|---|---|---|
| Common modules | sfhdelayedbq | tau_main | from 1 Myrs to 13 500 Myrs with a 500 Myrs step ; 30 000 |
| age_main | from 100 Myrs to 13 600 Myrs with a 100 Myrs step | ||
| age_bq [Myrs] | 1, 3, 5, 7, 10, 15, 20, 30, 40, 60, 80, 100, 150 | ||
| r_sfr | 0.01, 0.05, 0.1, 0.5, 1, 5, 10, 100 | ||
| nebular | logU | -2.0 | |
| zgas | 0.02, 0.008* | ||
| dustatt_modified_CF00 | Av_ISM | 24 linearly spaced values from 0.0 to 3.0 mag | |
| mu | 0.2, 0.3, 0.4, 0.5 | ||
| redshifting | redshift | – | |
| Stellar population modules | bc03 | imf | 0 (Salpeter) |
| metallicity | 0.02, 0.008* | ||
| separation_agea [Myrs] | 10 | ||
| cb19 | imf | 0 (Salpeter) | |
| metallicity | 0.02, 0.008* | ||
| upperb [Myrs] | 100 | ||
| separation_agea [Myrs] | 10 | ||
| bpass | imf | 2 (Salpeter) | |
| metallicity | 0.02, 0.008* | ||
| binary | 0, 1* | ||
| separation_agea [Myrs] | 10 | ||
Notes. Parameters that are not shown in the table were left at their default values.
Kept fixed for each individual run, but all given values were fit in separate runs.
The separation between the old and young stellar population.
The upper-mass cutoff of the IMF. This is a parameter only for the CB19 model and is left to the default value of 100 Myrs to match the assumed value in the other models.
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