RTGen applies post-processing Monte Carlo radiative transfer to six hydrodynamic galaxy simulations to compute dust temperatures, SEDs, continuum images, and molecular line emission while testing the effects of dust modeling choices.
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Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
RTGen applies post-processing Monte Carlo radiative transfer to six hydrodynamic galaxy simulations to compute dust temperatures, SEDs, continuum images, and molecular line emission while testing the effects of dust modeling choices.