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We present an effective system for simulating dust continuum observations byradiative transfer simulations. By using workflow management system RENKEI-WFT,we utilized distributed computing resources and automated a sequence ofcomputational tasks required for radiative transfer modeling, namely, mainradiative transfer simulations, pre-/post-processes, and data transfer betweencomputing resources. Our system simultaneously executes a lot of radiativetransfer simulations with different input parameters on distributed computingresources. This capability of our system enables us to conduct effectiveresearch by radiative transfer simulation. As a demonstration of our system, wesimulated dust continuum observations of protoplanetary disk. We performedhydrodynamic simulation modeling photoevaporating protoplanetary diskirradiated by ultra violet radiation from nearby massive stars. Results of thishydrodynamic simulation were used as input data for radiative transfersimulations. Expected spectral energy distributions and intensity maps wereobtained by our system.

Effective System for Simulating Dust Continuum Observations on Distributed Computing Resources