sunbather documentation

Welcome to the sunbather docs! On the left side, you’ll find the table of contents.

• Installing sunbather
  • Option 1: Installation with pip
  • Option 2: compilation from source
  • Post-installation steps
  • Testing your sunbather installation
  • Getting started with sunbather
• Glossary
  • The sunbather modules:
  • The $SUNBATHER_PROJECT_PATH
  • The planets.txt file
  • Stellar SED handling
• FAQ
  • How do I create Parker wind profiles?
  • How do I choose the composition of the atmosphere?
  • How do I calculate the transmission spectrum?
  • How do I simulate one planet with different stellar SEDs?
  • Why do I have to specify a pdir and a workingdir?
  • How do I read / plot the output of Cloudy in Python?
  • Can I run a Parker wind profile through Cloudy while using the isothermal temperature profile?
  • I forgot to specify some species for which I want Cloudy output with the save_sp argument. Do I need to run convergeT_parker.run() again from scratch?
  • Can I run an atmospheric profile other than an (isothermal) Parker wind?
  • How do I stop the simulation at the Roche radius / choose the maximum radius?
• API
  • sunbather
• Example: Fit Helium
  • License
  • Scientific goal
  • Methodology
  • Preparation
  • Function definitions
  • Retrieval of a mock spectrum of a hot Neptune
  • Retrieval of the observed helium spectrum of TOI-2134 b
• Example: Predict UV
  • License
  • Example goal
  • Example layout
  • Preparation
  • Step 1: Create Parker wind profiles with p-winds/Cloudy
  • Step 2: Run the Parker wind profiles through Cloudy
  • Step 3: Make NUV transit spectra
  • References