Fig. 27.

Zodiacal emissivities as a function of wavelength, combining IRAS, DIRBE, and Planck-HFI data. For reference, the dotted and dashed lines show emissivities that are unity at wavelengths less than 150 μm, and proportional to λ−2, λ−1, and λ0 at longer wavelengths. The emissivities for the cloud and the bands are very similar in level to those reported in HFImaps2015, but have smaller errors and show a smoother behaviour.
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