- 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

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