light_source_spectrum_file = 'spectrum_BTSettl_6200K_logg4.5_met0.dat' ! spectrum of the light sourcetarget
```
```
6. As a starting point, we will use a metallicity of 1 times the solar metallicity, no cloud, and a fixed eddy diffusion coefficient. Because of the effective temperature of the planet, TiO, VO and FeH are unlikely to have significant absorptions, so we will remove them in order to speed-up the calculations:
6. As a starting point, we will use a metallicity of 1 times the solar metallicity, no cloud, and a fixed eddy diffusion coefficient. Because of the effective temperature of the planet, TiO, VO and FeH are unlikely to have significant absorptions, so we will remove them in order to speed-up the calculations:
```text
```text
...
@@ -99,13 +93,13 @@ The figures should be in the _outputs/figures_ directory.
...
@@ -99,13 +93,13 @@ The figures should be in the _outputs/figures_ directory.
The temperature profile figure (temperature_profile_corot-4b) should look like this:
The temperature profile figure (temperature_profile_corot-4b) should look like this: