Getting-started.md

@@ -59,7 +59,7 @@ Copy and edit the file _inputs/example.nml_, rename it _corot-4b.nml_. An extend
     light_source_radius = 814e6  ! (m) radius of the light source
     light_source_range = 13.5e9  ! (m) distance between the target and the light source
     light_source_effective_temperature = 6190  ! (K) light source effective temperature 
-    ```text
+    ```
 5. 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
     metallicity = 1.0  ! (solar metallicity) atmospheric metallicity