Open Access

Fig. 10.

image

Variation of the solar dipole parameters (in rows) for different frequency bands (in columns) as a function of the Galactic mask in which the dipole is fitted. The black lines and gray band uncertainties show the final results of this work, using the Bcsep CMB anisotropies map. For reference, the pink lines and bands show the HFI-Legacy measurements. The four Planck Legacy CMB anisotropies maps are also tested, and are shown color coded.

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