Table 3.
Input parameters for the PARSEC model isochrones and corresponding luminosity functions.
| Option | Input | Default? |
|---|---|---|
| PARSEC version | 1.2S | Yes |
| COLIBRI version | S_35 | Yes |
| ninTPC | 10 | Yes |
| ηReimers | 0.2 | Yes |
| Photometric system | Gaia DR2, cf. Maíz Apellániz & Weiler (2018) | No |
| Bolometric corrections | YBC | Yes |
| Circumstellar dust | All left as default | Yes |
| Extinction | AV = 0 mag | Yes |
| Initial mass function | Chabrier (2001) for 0.1 ≤ M/M⊙ ≤ 1 | No |
| Salpeter (1955) for M/M⊙ > 1 | ||
| Ages | Linear age grid 1 Myr–70 Myr, step 0.5 Myr | No |
| Metallicities | Z = 0.0152; fixed. | Yes |
| Output 1 | Luminosity function, range −5 to 15 mag; bins 0.5 mag wide | No |
| Output 2 | Isochrones | Yes |
Notes. Parameters related to post-main sequence evolution are left as default values as they do not impact the results of this work. The parameter defaults only apply to version 3.3 of the CMD web tools; any updates of the web page may change the default options. ninTPC is the resolution of the thermal pulse cycles in the COLIBRI section (see Marigo et al. 2017); ηReimers is the parameter of mass loss on the RGB using the Reimers formula; YBC refers to the bolometric correction database by Chen et al. (2019).
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