The following papers are available:

• A 3D radiative transfer framework: I. non-local operator splitting and continuum scattering problems
• A 3D radiative transfer framework: II. line transfer problems
• A 3D radiative transfer framework: III. periodic boundary conditions
  
• The Limiting Effects of Dust in Brown Dwarf Model Atmospheres
  
• Parallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program. III: A parallel algorithm for direct opacity sampling
  
• Spherically symmetric model atmospheres for low mass pre-Main Sequence stars with effective temperatures between 2000 and 6800K
  
• The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800K
  
• The NextGen Model Atmosphere grid
  
• Numerical Solution of the Expanding Stellar Atmosphere Problem
  
• Parallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program. II: Wavelength Parallelization
  
• Parallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program