Generic Grid


Based on the generic ATMO grid presented in Goyal et al. (2018). Using the model grid as a framework, we allow you to rescale your models with custom temperature, gravity, and radius values.

\(\small \text{K}\)
The temperature (in Kelvin) of the planet.
\(\small \text{$\frac{m}{s^2}$}\)
The gravity (in \(\small \text{$\frac{meters}{second^2}$}\)) of the planet.
\(\small \text{Jupiter radius}\)
The radius of the planet (normalized to Jupiter).
\(\small \text{Solar radius}\)
The radius of the star (normalized to the sun).
Rainout condensation assumes material which condenses is depleted from all layers of the model in the condensate forming layer and above. Local condensation assumes material which condenses is depleted independently in each layer of the model atmosphere.
Metallicity in solar units.
The Carbon to Oxygen ratio. (Note that solar is 0.56.)
Wavelength dependent scattering opacity. 1 corresponds to normal scattering whereas 1100 corresponds to enhanced scattering from the optical to IR.
Uniform scattering opacity with cut off at all wavelengths. 0.0 corresponds to no clouds, 1.0 corresponds to full clouds.


Results




One of the parameters to make up the model was missing or out of range. Above is a fun demonstration of what your model could have looked like!

The closest match used for your rescale was :

temperature gravity
your input
model parameter 400 50

References

Jayesh M Goyal, Hannah R Wakeford, Nathan J Mayne, Nikole K Lewis, Benjamin Drummond, David K Sing; Fully scalable forward model grid of exoplanet transmission spectra, Monthly Notices of the Royal Astronomical Society, Volume 482, Issue 4, 1 February 2019, Pages 4503–4513, https://doi.org/10.1093/mnras/sty3001