Tutorial

• Getting Started
  • Preparing a radiative transfer object
  • Calculating a transmission spectrum
  • Calculating an emission spectrum
  • An alternative: the SpectralModel object
• High-resolution spectra
  • Transmission spectrum
  • Emission Spectrum
• Including clouds
  • Gray cloud deck
  • Scaled Rayleigh scattering
  • Powerlaw cloud models
  • Condensate clouds from real optical constants
  • Defining arbitrary opacity functions (can be used to parameterize clouds)
  • Cloud fraction
  • Emission spectra
  • SpectralModel
• Scattering for Emission Spectra
  • Self-scattering in gas giants
  • Scattering of stellar light
  • Geometries
  • Surface scattering
• Analysis tools
  • Transmission contribution functions
  • Emission contribution functions
  • Plotting opacity contributions
  • Plotting opacities
  • Getting mettalicity and elemental abundances from mass fractions
• Retrieval Examples
  • Retrievals: Basic Retrieval Tutorial
  • Retrievals: Dealing with multiple datasets
  • Retrievals: Emission Spectra Retrieval
  • Retrievals: Exploring the built-in models
  • JWST retrieval workflow with SpectralModel
  • High-resolution retrieval workflow with SpectralModel
• SpectralModel
  • Introduction
  • Basic usage
  • Calculating a transmission spectrum
  • Calculating an emission spectrum
  • Calculating a time-varying high-resolution spectrum
  • Built-in functions
  • Spectral modifications in details
  • Tellurics, deformations, and noise
  • Preparing ground-based high-resolution spectra
  • Saving and loading
  • Modifying the model functions and the spectral modification functions
  • Useful tips
• Planet: a convenient way to access planetary data
  • Getting Planet data
  • Basic Planet usage
  • Other useful function
  • Loading and saving
  • Plotting the planet’s mass and radius in context to other exoplanets
• Rebinning opacities
  • Binning opacities in c-k mode
  • Downsampling lbl opacities
  • Wavelength binning vs. spectral resolution
• Utility functions
  • Constants
  • Planck function
  • PHOENIX and ATLAS9 stellar model spectra
  • Guillot temperature model
• Interpolating chemical equilibrium abundances
  • Example