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