Markov Chain Monte Carlo (MCMC) Analysis of Phase Curve Models and Observational Data for Exoplanets

Predefine Lambert sacttering, specular reflection and atmospheric scattering models.

Inputs

• Phase curve model: Spectral model: ./core; Lambert model: ./core_lambert
• Observation target: Defined in: parameters.py, Sampling.py
• Observation data: Kepler data for the target K2-141 b
• Prior distribution of parameters

Attention

• Read and follow ./check_list.py to verify settings after changing the target.

Outputs

• Posterior distribution of parameters