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. Author manuscript; available in PMC: 2021 Oct 12.
Published in final edited form as: Astrophys J. 2015 Jul 9;807(2):161. doi: 10.1088/0004-637x/807/2/161

Figure 20.

Figure 20.

Difference of the filtered dust residual map from the last iteration minus the map from iteration zero, divided by the former. We show as an example in ROI A the case for which the radiance map R is considered and the errors in the definition of the χ2 are assumed to be proportional to M as defined in Equation (4). The map is shown in the plate carrée projection used in the dust and γ-ray fits for ROI A, and the magenta line shows the border of the region considered in the fit.