Table 1.
Stellar atmosphere models used for the benchmarking of our code.
| Model ID | Teff (K) | log g (cm s−2) | Radius (R⊙) | ξ (km s−1) | LTE |
|---|---|---|---|---|---|
| sun | 5777 | 4.44 | 1.00 | 1 | Yes |
| s8000 | 8000 | 2.50 | 9.34 | 1 | Yes |
| s3500 | 3500 | 3.50 | 2.95 | 2 | Yes |
| C | 5777 | 4.44 | 1.00 | variable | No |
Notes. Models are taken from the MARCS database and correspond to the photosphere, except the model C taken from Fontenla et al. (1999). The first column indicates the designation of the model; the second, third, and fourth are the effective temperature, log surface gravity, and radius of the star, respectively. The fifth column gives the constant microturbulence, except for the FAL-C model, which has a depth varying microturbulence. The last column indicates if the model is computed assuming LTE.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.