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. Author manuscript; available in PMC: 2021 Oct 12.
Published in final edited form as: Astrophys J. 2017 Aug 31;846(1):67. doi: 10.3847/1538-4357/aa844d

Figure 4.

Figure 4.

Longitude profile averaged over −5° < 5 < b° for the modified SKY (left, R12) and COBE/DIRBE bar/disk (right, F98) models. Colored curves show the data for COBE/DIRBE and reprocessed IRAS, while black lines show the model predictions convolved with the instrumental bandpass overlaid on the data for the COBE/DIRBE 2.2 μm (solid) and 4.9 μm (long-dashed) and the IRAS 25 μm (long-dashed–dotted), 60 μm (long-dashed–double-dotted), and 100 μm (long-dashed–triple-dotted) bands.