Table 5: Residuals between the model and the observation. For each COBE/DIRBE map we present the percentage of the Galaxy's area with residuals less than <10%, <20%, and <50%.
Wavelength ( $\mu$ m) <10% <20% <50%

1.2 29% 53% 92%

2.2 32% 55% 87%

60 26% 52% 88%

100 23% 43% 81%

140 28% 51% 81%

240 18% 37% 75%

HI 17% 38% 85%

H₂ 17% 35% 67%

**Table 5:** Residuals between the model and the observation. For each COBE/DIRBE map we present the percentage of the Galaxy's area with residuals less than <10%, <20%, and <50%.
Wavelength ( $\mu$ m)	<10%	<20%	<50%
1.2	29%	53%	92%
2.2	32%	55%	87%
60	26%	52%	88%
100	23%	43%	81%
140	28%	51%	81%
240	18%	37%	75%
HI	17%	38%	85%
H₂	17%	35%	67%

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