| Tom Abel | KIPAC, Menlo Park | USA | Talk |
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Radiation Transport in 3D AMR Simulations of Star Formation in the Galaxy |
| Maarten Baes | Sterrenkundig Observatorium, Universiteit Gent | Belgium | Talk |
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Benchmarking continuum LTE radiative transfer codes in a disc galaxy environment |
| Tom Bethell | Department of Astronomy, University of Michigan | USA | Talk |
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Monte Carlo and the Delaunay Tesselation: radiative transfer on an unstructured and adaptive grid |
| Simone Bianchi | IR/CNR, Firenze | Italy | Talk |
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Radiative transfer in a clumpy galactic disk |
| Sukanya Chakrabarti | Harvard-Smithsonian CfA | USA | Talk |
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RADISHE'ing Simulations - from Protostars to Galaxies |
| Cornelis Dullemond | MPIA Heidelberg | Germany | Talk |
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Radiative transfer with quantum heated grains |
| Barbara Ercolano | Institute of Astronomy, University of Cambridge | UK | Talk |
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3D photoionisation and dust RT calculations with Monte Carlo methods |
| Kristian Finlator | Department of Astronomy, University of Arizona | USA | Talk |
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Accuracy and Speed in Moment Methods for Continuum Radiative Transfer |
| Bernd Freytag | ENS, Lyon | France | Talk |
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Radiation hydrodynamics simulations of dust layers in brown dwarfs |
| Karl Gordon | Steward Observatory, Tucson | USA | Talk |
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Radiative transfer in DIRTY and the DIRTY view of Star Formation Rate Indicators |
| Ilian Iliev | University of Zurich | Switzerland | Talk |
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Simulating Reionization at Large Scales |
| Patrik Jonsson | University of California, Santa Cruz | USA | Talk PDF 3.1MB Poster PDF 2.5MB |
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Polychromatic Radiative Transfer with Sunrise |
| Mika Juvela | Helsinki University Observatory | Finnland | Talk |
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Radiative transfer on AMR grids |
| Eric Keto | Harvard-Smithsonian Center for Astrophysics | USA | Talk |
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Modeling non-LTE hyperfine emission |
| Chael Kruip | Huygens Laboratory Leiden | The Netherlands | Talk 2.5MB |
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| Michiel Min | Astronomical Institute 'Anton Pannekoek' | The Netherlands | Talk |
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Radiative transfer in massive protoplanetary disks |
| Karl Misselt | Steward Observatory, University of Arizona, Tuscon | USA | Talk |
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| Aake Nordlund | Niels Bohr Institute Copenhagen | Denmark | Talk |
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Fast radiative transfer for MPI and AMR |
| Yaroslav Pavlyuchenkov | MPIA Heidelberg | Germany | Talk |
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Molecular Line Radiative Transfer in Prestellar Objects |
| Christophe Pinte | University of Exeter | UK | Talk |
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Multi-wavelength modelling of protoplanetary disks |
| Thomas Robitaille | St. Andrews | UK | Talk |
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Radiation transfer modeling of young stars |
| Ralf Siebenmorgen | ESO Garching | Germany | Talk PDF 0.3MB |
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T Tauri disk emission and PAH destruction |
| Dimitris Stamatellos | Cardiff University, Cardiff | UK | Talk |
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Radiative transfer in starless clouds and young embedded protostars |
| Jürgen Steinacker | MPIA Heidelberg | Germany | Talk |
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Ray-tracing applied to star formation: inverse radiative transfer, high optical depths, resolution issues, and fitting algorithms |
| Richard Tuffs | MPIK Heidelberg | Germany | Talk |
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Calculation of radiation fields in galaxies using the method of scattered intensities |
| Nikolai Voshchinnikov | Sobolev Astronomical Institute, St. Petersburg University | Russia | Talk |
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How large speculations allow us light scattering theory? |
| Rainer Wehrse | ITA Heidelberg | Germany | Talk |
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Markov process simulations for radiative transfer problems |
| Barbara Whitney | Space Science Institute | USA | Talk |
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Full Treatment of Polarization: Emission, Scattering, Aligned Grains, Arbitrary Magnetic Fields, Multi-Wavelength |
| John Wise | NASA/GSFC | USA | Talk |
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Adaptive Ray Tracing in AMR Radiation Hydrodynamics Simulations |
| Sebastian Wolf | Kiel University | Germany | Talk PDF 4.4MB |
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Monte Carlo RT in Planet Formation Studies; Astrophysics Software Database |
| Michael Wolff | Space Science Institute | USA | Talk |
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Validity of the plane-parallel approximation and corrections to perform radiative transfer in curved atmospheres |
| Manolis Xilouris
Nick Kylafis |
National Observatory of Athens, Athens | Greece | Talk |
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3D Radiative transfer models of spiral galaxies: The method of scattered intensities |





















