-orange){kind=icon}
Differentiable spectral modelling of exoplanets/brown dwarfs/M dwarfs using JAX! Read the docs 🐕. In short, ExoJAX allows you to do gradient based optimizations, HMC-NUTS, and SVI using the latest database.
ExoJAX is at least compatible with
ExoJAX Classes
- Databases: *db (mdb: molecular, adb: atomic, cdb:continuum, pdb: particulates)
- Opacity Calculators: opa (Voigt profile, CIA, Mie, Rayleigh scattering etc)
- Atmospheric Radiative Transfer: art (emission w, w/o scattering, refelction, transmission)
- Spectral Operator: sop (planet rotation, instrumental boradening)
- Atompsheric Microphysics: amp (clouds etc)
See this page for the first step!
- ⭐ exojaxample_WASP39b : An example of HMC-NUTS for actual hot Saturn (JWST/ERS, NIRSPEC/G395H)
- ⭐ exojaxample_jupiter : An example of HMC-NUTS for actual Jupiter reflection spectrum
-orange){kind=icon}
- Paper I: Kawahara, Kawashima, Masuda, Crossfield, Pannier, van den Bekerom, ApJS 258, 31 (2022)
- Paper II: in prep
🐈 Copyright 2020-2024 ExoJAX contributors. ExoJAX is publicly available under the MIT license.