Fig. 3

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Predicted dust densities and temperatures for a single example cube slice perpendicular to the LoS. A comparison between the three point estimation methods to the ground truth is shown in the left column. The top two rows give the 23-wavelength SLoS-cINN result for the ISRF-only scenario, while rows 3 and 4 display the counterpart for the ISRF + star case. Rows 5 and 6 present the NLoS-based outcome for the ISRF-only case, and the last two rows show the corresponding seven wavelengths SLoS-cINN prediction. The listed NRMSE and median absolute relative errors are averages over this slice only and not the entire cube.
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